{"help":"Return the metadata of a dataset (package) and its resources. :param id: the id or name of the dataset :type id: string","success":true,"result":[{"id":"89553198-d185-4541-9ea3-456a581d6cb5","name":"space-resolved-gas-temperature-microwave-plasma-torch-used-hydrogen-production-methane","title":"Space resolved gas temperature of a microwave plasma torch used for hydrogen production via methane pyrolysis","author_email":"Simon.Kreuznacht@ruhr-uni-bochum.de","maintainer":"Research Data Repository","maintainer_email":"achim.vonkeudell@rub.de","license_title":"https:\/\/creativecommons.org\/licenses\/by\/4.0\/","notes":"\u003Cp\u003EPyrolysis of methane is a promising, new, greenhouse gas-free production method of hydrogen. Here, we present optical emission spectra of a microwave plasma torch operated in an argon methane mixture. Detailed spatial resolution is achieved by means of Abel inversion. The emission spectra are dominated by dicarbon Swan bands and black body radiation from carbon nanoparticles. Both spectral features are utilized to estimate the gas temperature. In the center of the plasma, gas temperatures of up to 4300 K are reached with large gradients (500 K\/mm) in radial direction. The thermal equilibrium chemistry and the kinetics of methane pyrolysis are analyzed to explain the observed coupling between the local gas temperature and the local emission.\u003C\/p\u003E\n","url":"https:\/\/rdpcidat.rub.de\/dataset\/space-resolved-gas-temperature-microwave-plasma-torch-used-hydrogen-production-methane","state":"Active","log_message":"Update to resource Figure C3b_NMSSE between two simulated spectra as a function of the rotational temperature and the full width at half maximum Delta v=1","private":true,"revision_timestamp":"Tue, 06\/10\/2025 - 10:04","metadata_created":"Tue, 04\/09\/2024 - 15:41","metadata_modified":"Tue, 06\/10\/2025 - 10:04","creator_user_id":"0230e7f1-41c9-46b9-85f6-e08ce6928190","type":"Dataset","resources":[{"id":"42fe3f24-953e-4993-a781-64eaba76183c","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%202_Uncalibrated%20overview%20spectrum.txt","description":"\u003Cp\u003EUncalibrated overview spectrum of the emission from the microwave plasma torch (MPT).\u003C\/p\u003E\n","format":".txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure 2_Uncalibrated overview spectrum","mimetype":"text\/plain","size":"13.9 KB","created":"Tue, 06\/10\/2025 - 09:37","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"320072dc-d726-4c3f-ae72-8e3f020b47a0","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%203_Radially%20resolved%20amplitudes%20and%20temperatures.txt","description":"\u003Cp\u003ERadially resolved measured values for the amplitudes of the black body radiation and the dicarbon Swan bands emission as well as the formally fitted temperature of the black body radiation and the fitted rotational temperature of the dicarbon molecules at the axial position z=5 mm for operating parameter set 1 (compare Table 1). The resulting gas temperature determined from the two fitted temperatures is also shown.\u003C\/p\u003E\n","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure 3_Radially resolved amplitudes and temperatures","mimetype":"text\/plain","size":"2.78 KB","created":"Tue, 06\/10\/2025 - 09:38","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"5d1ae8fb-6bc0-442b-bc7e-58ba23619811","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%204a_Space%20resolved%20gas%20temperature%2060%20slm%2C%204%25%20CH4%2C%20900%20W.txt","description":"","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure 4a_Space resolved gas temperature 60 slm, 4% CH4, 900 W","mimetype":"text\/plain","size":"5.38 KB","created":"Tue, 06\/10\/2025 - 09:39","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"18c0ca0f-4be7-4ba4-b366-887e5a6dbb20","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%204b_Space%20resolved%20gas%20temperature%2060%20slm%2C%204%25%20CH4%2C%201800%20W.txt","description":"","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure 4b_Space resolved gas temperature 60 slm, 4% CH4, 1800 W","mimetype":"text\/plain","size":"5.97 KB","created":"Tue, 06\/10\/2025 - 09:39","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"39e5cf3a-5059-4415-9a52-7eacf14eaef6","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%204c_Space%20resolved%20gas%20temperature%2060%20slm%2C%208%25%20CH4%2C%201800%20W.txt","description":"","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure 4c_Space resolved gas temperature 60 slm, 8% CH4, 1800 W","mimetype":"text\/plain","size":"5.69 KB","created":"Tue, 06\/10\/2025 - 09:40","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"a7d26049-dbda-4d0f-9240-f31721f08e22","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%204d_Space%20resolved%20gas%20temperature%2080%20slm%2C%204%25%20CH4%2C%201200%20W.txt","description":"","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure 4d_Space resolved gas temperature 80 slm, 4% CH4, 1200 W","mimetype":"text\/plain","size":"5.45 KB","created":"Tue, 06\/10\/2025 - 09:40","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"4e37fe2e-fd16-4e24-9ffa-7d8bad58d026","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%205a_Space%20resolved%20dicarbon%20Swan%20Bands%20emission%20amplitude%2060%20slm%2C%204%25%20CH4%2C%20900%20W.txt","description":"","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure 5a_Space resolved dicarbon Swan Bands emission amplitude 60 slm, 4% CH4, 900 W","mimetype":"text\/plain","size":"5.54 KB","created":"Tue, 06\/10\/2025 - 09:40","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"69f88a30-787f-4e3d-be9c-464c406bd71a","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%205b_Space%20resolved%20dicarbon%20Swan%20Bands%20emission%20amplitude%2060%20slm%2C%204%25%20CH4%2C%201800%20W.txt","description":"","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure 5b_Space resolved dicarbon Swan Bands emission amplitude 60 slm, 4% CH4, 1800 W","mimetype":"text\/plain","size":"5.49 KB","created":"Tue, 06\/10\/2025 - 09:40","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"c2aa33b8-f803-445b-8e0b-20e1d3698250","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%205c_Space%20resolved%20dicarbon%20Swan%20Bands%20emission%20amplitude%2060%20slm%2C%208%25%20CH4%2C%201800%20W.txt","description":"","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure 5c_Space resolved dicarbon Swan Bands emission amplitude 60 slm, 8% CH4, 1800 W","mimetype":"text\/plain","size":"5.55 KB","created":"Tue, 06\/10\/2025 - 09:40","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"8f65ada3-8a9b-4490-bfb1-d9ce357619c0","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%205d_Space%20resolved%20dicarbon%20Swan%20Bands%20emission%20amplitude%2080%20slm%2C%204%25%20CH4%2C%201200%20W.txt","description":"","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure 5d_Space resolved dicarbon Swan Bands emission amplitude 80 slm, 4% CH4, 1200 W","mimetype":"text\/plain","size":"5.56 KB","created":"Tue, 06\/10\/2025 - 09:41","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"8374736c-1fd6-45c0-9e70-ad13765d1981","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%206a_Space%20resolved%20black%20body%20emission%20amplitude%2060%20slm%2C%204%25%20CH4%2C%20900%20W.txt","description":"","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure 6a_Space resolved black body emission amplitude 60 slm, 4% CH4, 900 W","mimetype":"text\/plain","size":"5.65 KB","created":"Tue, 06\/10\/2025 - 09:41","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"fce71e97-5bd2-4f43-9fa9-282b72d0747f","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%206b_Space%20resolved%20black%20body%20emission%20amplitude%2060%20slm%2C%204%25%20CH4%2C%201800%20W.txt","description":"","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure 6b_Space resolved black body emission amplitude 60 slm, 4% CH4, 1800 W","mimetype":"text\/plain","size":"5.68 KB","created":"Tue, 06\/10\/2025 - 09:41","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"a864625f-335f-4928-8b2b-7f6403c365d9","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%206c_Space%20resolved%20black%20body%20emission%20amplitude%2060%20slm%2C%208%25%20CH4%2C%201800%20W.txt","description":"","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure 6c_Space resolved black body emission amplitude 60 slm, 8% CH4, 1800 W","mimetype":"text\/plain","size":"5.65 KB","created":"Tue, 06\/10\/2025 - 09:41","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"a7577971-32a4-430c-9c72-405197de10d1","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%206d_Space%20resolved%20black%20body%20emission%20amplitude%2080%20slm%2C%204%25%20CH4%2C%201200%20W.txt","description":"","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure 6d_Space resolved black body emission amplitude 80 slm, 4% CH4, 1200 W","mimetype":"text\/plain","size":"5.66 KB","created":"Tue, 06\/10\/2025 - 09:42","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"6eadd106-1954-4542-9743-d1416bfea582","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%207_Thermal%20equilibrium%20mole%20fractions.txt","description":"\u003Cp\u003EMole fractions of hydrogen, dicarbon, methane, and solid carbon in thermal equilibrium as a function of gas temperature for the pyrolysis of 4%vol methane in argon at atmospheric pressure.\u003C\/p\u003E\n","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure 7_Thermal equilibrium mole fractions","mimetype":"text\/plain","size":"189.54 KB","created":"Tue, 06\/10\/2025 - 09:42","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"1203b1b0-d9ba-41d2-8eee-fbfb0f622494","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%208a_Methane%20Pyrolysis%20Kinetics%20at%201400%20K.txt","description":"\u003Cp\u003EComparison of the kinetics of methane pyrolysis at a pressure of 1\u2009atm and pure methane as initial condition according to the full mechanism of Fincke et al. and according to the simplified mechanism with optimized rate constants at a gas temperature of 1400 K.\u003C\/p\u003E\n","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure 8a_Methane Pyrolysis Kinetics at 1400 K","mimetype":"text\/plain","size":"78.08 KB","created":"Tue, 06\/10\/2025 - 09:44","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"ebbadc90-5f2a-4a7a-a18b-53e3e797bafb","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%208b_Methane%20Pyrolysis%20Kinetics%20at%202100%20K.txt","description":"\u003Cp\u003EComparison of the kinetics of methane pyrolysis at a pressure of 1\u2009atm and pure methane as initial condition according to the full mechanism of Fincke et al. and according to the simplified mechanism with optimized rate constants at a gas temperature of 2100 K.\u003C\/p\u003E\n","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure 8b_Methane Pyrolysis Kinetics at 2100 K","mimetype":"text\/plain","size":"97.93 KB","created":"Tue, 06\/10\/2025 - 09:45","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"31a92040-bf19-470d-aa04-9d2666ee5a41","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%208c_Methane%20Pyrolysis%20Kinetics%20at%203600%20K.txt","description":"\u003Cp\u003EComparison of the kinetics of methane pyrolysis at a pressure of 1\u2009atm and pure methane as initial condition according to the full mechanism of Fincke et al. and according to the simplified mechanism with optimized rate constants at a gas temperature of 3600 K.\u003C\/p\u003E\n","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure 8c_Methane Pyrolysis Kinetics at 3600 K","mimetype":"text\/plain","size":"131.79 KB","created":"Tue, 06\/10\/2025 - 09:45","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"4d0ae83a-472d-455e-b39f-198ae8ecfcb2","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%20C1a_Simulated%20dicarbon%20Swan%20bands%20Delta%20v%3D2.txt","description":"\u003Cp\u003ESimulated spectrum of the Delta v=2 band sequence of the dicarbon Swan bands. Trot=Tvib=4000 K; Gaussian line profile with a full width at half maximum of 50 pm.\u003C\/p\u003E\n","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure C1a_Simulated dicarbon Swan bands Delta v=2","mimetype":"text\/plain","size":"31.35 KB","created":"Tue, 06\/10\/2025 - 09:47","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"8b9ef1a1-3f83-4a29-a0b6-4f583822d43c","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%20C1b_Simulated%20dicarbon%20Swan%20bands%20Delta%20v%3D1.txt","description":"\u003Cp\u003ESimulated spectrum of the Delta v=1 band sequence of the dicarbon Swan bands. Trot=Tvib=4000 K; Gaussian line profile with a full width at half maximum of 50 pm.\u003C\/p\u003E\n","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure C1b_Simulated dicarbon Swan bands Delta v=1","mimetype":"text\/plain","size":"30.91 KB","created":"Tue, 06\/10\/2025 - 09:48","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"ac4a6143-e654-403c-a490-bac6f86769d2","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%20C1c_Simulated%20dicarbon%20Swan%20bands%20Delta%20v%3D0.txt","description":"\u003Cp\u003ESimulated spectrum of the Delta v=0 band sequence of the dicarbon Swan bands. Trot=Tvib=4000 K; Gaussian line profile with a full width at half maximum of 50 pm.\u003C\/p\u003E\n","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure C1c_Simulated dicarbon Swan bands Delta v=0","mimetype":"text\/plain","size":"31.04 KB","created":"Tue, 06\/10\/2025 - 09:48","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"61159499-67d1-4f9b-906a-12ee49450238","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%20C1d_Simulated%20dicarbon%20Swan%20bands%20Delta%20v%3D-1.txt","description":"\u003Cp\u003ESimulated spectrum of the Delta v=-1 band sequence of the dicarbon Swan bands. Trot=Tvib=4000 K; Gaussian line profile with a full width at half maximum of 50 pm.\u003C\/p\u003E\n","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure C1d_Simulated dicarbon Swan bands Delta v=-1","mimetype":"text\/plain","size":"30.86 KB","created":"Tue, 06\/10\/2025 - 09:49","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"c6267e4b-bbf6-4771-af12-f782d2d953c7","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%20C1e_Simulated%20dicarbon%20Swan%20bands%20Delta%20v%3D-2.txt","description":"\u003Cp\u003ESimulated spectrum of the Delta v=-2 band sequence of the dicarbon Swan bands. Trot=Tvib=4000 K; Gaussian line profile with a full width at half maximum of 50 pm.\u003C\/p\u003E\n","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure C1e_Simulated dicarbon Swan bands Delta v=-2","mimetype":"text\/plain","size":"30.91 KB","created":"Tue, 06\/10\/2025 - 09:50","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"586a8632-f60a-436f-b733-cb3bc073068d","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%20C2_NMSSE%20between%20two%20simulated%20spectra%20as%20a%20function%20of%20the%20rotational%20temperature.txt","description":"\u003Cp\u003ENMSSE between two simulated spectra of the five band sequences of the dicarbon Swan bands as a function of the rotational temperature of the second spectrum. The first spectrum has a rotational temperature of 4000\u2009K. Solely on the basis of the typical experimental signal-to-noise ratio a NMSSE of around 2.5 x 10^-7 is expected.\u003C\/p\u003E\n","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure C2_NMSSE between two simulated spectra as a function of the rotational temperature","mimetype":"text\/plain","size":"19.8 KB","created":"Tue, 06\/10\/2025 - 09:54","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"c9f7dc74-49c8-4e3b-9fba-770c8f4423a5","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%20C3a_NMSSE%20between%20two%20simulated%20spectra%20as%20a%20function%20of%20the%20rotational%20temperature%20and%20the%20full%20width%20at%20half%20maximum%20Delta%20v%3D2.txt","description":"\u003Cp\u003ENMSSE  between two simulated spectra of the Delta v=2 band sequence of the dicarbon Swan bands as a function of the rotational temperature and full width at half maximum of the line shape of the second spectrum. The first spectrum here has a rotational temperature of 4000\u2009K and a full width at half maximum of the line shape of 50\u2009pm. Solely on the basis of the typical experimental signal-to-noise ratio a NMSSE of around 2.5 x 10^-7 is expected.\u003C\/p\u003E\n","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure C3a_NMSSE between two simulated spectra as a function of the rotational temperature and the full width at half maximum Delta v=2","mimetype":"text\/plain","size":"1.05 MB","created":"Tue, 06\/10\/2025 - 09:55","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"a1b20108-d790-4c9b-93c9-1795cc3292b3","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%20C3b_NMSSE%20between%20two%20simulated%20spectra%20as%20a%20function%20of%20the%20rotational%20temperature%20and%20the%20full%20width%20at%20half%20maximum%20Delta%20v%3D1.txt","description":"\u003Cp\u003ENMSSE  between two simulated spectra of the Delta v=1 band sequence of the dicarbon Swan bands as a function of the rotational temperature and full width at half maximum of the line shape of the second spectrum. The first spectrum here has a rotational temperature of 4000\u2009K and a full width at half maximum of the line shape of 50\u2009pm. Solely on the basis of the typical experimental signal-to-noise ratio a NMSSE of around 2.5 x 10^-7 is expected.\u003C\/p\u003E\n","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure C3b_NMSSE between two simulated spectra as a function of the rotational temperature and the full width at half maximum Delta v=1","mimetype":"text\/plain","size":"1.05 MB","created":"Tue, 06\/10\/2025 - 09:56","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"a73614ea-e68b-42e2-bad6-21b0e536b321","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%20C3c_NMSSE%20between%20two%20simulated%20spectra%20as%20a%20function%20of%20the%20rotational%20temperature%20and%20the%20full%20width%20at%20half%20maximum%20Delta%20v%3D0.txt","description":"\u003Cp\u003ENMSSE  between two simulated spectra of the Delta v=0 band sequence of the dicarbon Swan bands as a function of the rotational temperature and full width at half maximum of the line shape of the second spectrum. The first spectrum here has a rotational temperature of 4000\u2009K and a full width at half maximum of the line shape of 50\u2009pm. Solely on the basis of the typical experimental signal-to-noise ratio a NMSSE of around 2.5 x 10^-7 is expected.\u003C\/p\u003E\n","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure C3c_NMSSE between two simulated spectra as a function of the rotational temperature and the full width at half maximum Delta v=0","mimetype":"text\/plain","size":"1.05 MB","created":"Tue, 06\/10\/2025 - 09:56","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"db53e489-c83f-4ce8-ba59-e3f2eaf8575d","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%20C3d_NMSSE%20between%20two%20simulated%20spectra%20as%20a%20function%20of%20the%20rotational%20temperature%20and%20the%20full%20width%20at%20half%20maximum%20Delta%20v%3D-1.txt","description":"\u003Cp\u003ENMSSE  between two simulated spectra of the Delta v=-1 band sequence of the dicarbon Swan bands as a function of the rotational temperature and full width at half maximum of the line shape of the second spectrum. The first spectrum here has a rotational temperature of 4000\u2009K and a full width at half maximum of the line shape of 50\u2009pm. Solely on the basis of the typical experimental signal-to-noise ratio a NMSSE of around 2.5 x 10^-7 is expected.\u003C\/p\u003E\n","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure C3d_NMSSE between two simulated spectra as a function of the rotational temperature and the full width at half maximum Delta v=-1","mimetype":"text\/plain","size":"1.05 MB","created":"Tue, 06\/10\/2025 - 09:56","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"7c131c02-f1f1-4ccf-9bfe-521092c86498","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%20C3e_NMSSE%20between%20two%20simulated%20spectra%20as%20a%20function%20of%20the%20rotational%20temperature%20and%20the%20full%20width%20at%20half%20maximum%20Delta%20v%3D-2.txt","description":"\u003Cp\u003ENMSSE  between two simulated spectra of the Delta v=-2 band sequence of the dicarbon Swan bands as a function of the rotational temperature and full width at half maximum of the line shape of the second spectrum. The first spectrum here has a rotational temperature of 4000\u2009K and a full width at half maximum of the line shape of 50\u2009pm. Solely on the basis of the typical experimental signal-to-noise ratio a NMSSE of around 2.5 x 10^-7 is expected.\u003C\/p\u003E\n","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure C3e_NMSSE between two simulated spectra as a function of the rotational temperature and the full width at half maximum Delta v=-2","mimetype":"text\/plain","size":"1.05 MB","created":"Tue, 06\/10\/2025 - 09:57","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"387402b2-edda-4534-b6b1-d4ab3fe99fa1","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%20C4a_NMSSE%20between%20two%20simulated%20spectra%20as%20a%20function%20of%20the%20rotational%20and%20vibrational%20temperatures%20Delta%20v%3D2.txt","description":"\u003Cp\u003ENMSSE  between two simulated spectra of the Delta v=2 band sequence of the dicarbon Swan bands as a function of the rotational and vibrational temperature of the second spectrum. The first spectrum has a rotational and vibrational temperature of 4000\u2009K. Solely on the basis of the typical experimental signal-to-noise ratio a NMSSE of around 2.5 x 10^-7 is expected.\u003C\/p\u003E\n","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure C4a_NMSSE between two simulated spectra as a function of the rotational and vibrational temperatures Delta v=2","mimetype":"text\/plain","size":"1.16 MB","created":"Tue, 06\/10\/2025 - 09:58","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"2ff1fb18-47ca-4ac5-84eb-944a15547c7f","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%20C4b_NMSSE%20between%20two%20simulated%20spectra%20as%20a%20function%20of%20the%20rotational%20and%20vibrational%20temperatures%20Delta%20v%3D1.txt","description":"\u003Cp\u003ENMSSE  between two simulated spectra of the Delta v=1 band sequence of the dicarbon Swan bands as a function of the rotational and vibrational temperature of the second spectrum. The first spectrum has a rotational and vibrational temperature of 4000\u2009K. Solely on the basis of the typical experimental signal-to-noise ratio a NMSSE of around 2.5 x 10^-7 is expected.\u003C\/p\u003E\n","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure C4b_NMSSE between two simulated spectra as a function of the rotational and vibrational temperatures Delta v=1","mimetype":"text\/plain","size":"1.11 MB","created":"Tue, 06\/10\/2025 - 09:59","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"225185cb-0c3e-468b-ae0e-3f48ea08cd01","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%20C4c_NMSSE%20between%20two%20simulated%20spectra%20as%20a%20function%20of%20the%20rotational%20and%20vibrational%20temperatures%20Delta%20v%3D0.txt","description":"\u003Cp\u003ENMSSE  between two simulated spectra of the Delta v=0 band sequence of the dicarbon Swan bands as a function of the rotational and vibrational temperature of the second spectrum. The first spectrum has a rotational and vibrational temperature of 4000\u2009K. Solely on the basis of the typical experimental signal-to-noise ratio a NMSSE of around 2.5 x 10^-7 is expected.\u003C\/p\u003E\n","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure C4b_NMSSE between two simulated spectra as a function of the rotational and vibrational temperatures Delta v=0","mimetype":"text\/plain","size":"1.16 MB","created":"Tue, 06\/10\/2025 - 09:59","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"6f6e08e1-6398-4d47-b9f8-3f0ca9f919da","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%20C4d_NMSSE%20between%20two%20simulated%20spectra%20as%20a%20function%20of%20the%20rotational%20and%20vibrational%20temperatures%20Delta%20v%3D-1.txt","description":"\u003Cp\u003ENMSSE  between two simulated spectra of the Delta v=-1 band sequence of the dicarbon Swan bands as a function of the rotational and vibrational temperature of the second spectrum. The first spectrum has a rotational and vibrational temperature of 4000\u2009K. Solely on the basis of the typical experimental signal-to-noise ratio a NMSSE of around 2.5 x 10^-7 is expected.\u003C\/p\u003E\n","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure C4d_NMSSE between two simulated spectra as a function of the rotational and vibrational temperatures Delta v=-1","mimetype":"text\/plain","size":"1.16 MB","created":"Tue, 06\/10\/2025 - 10:00","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"933707b5-75bb-415f-b92d-427f5092b5a4","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%20C4e_NMSSE%20between%20two%20simulated%20spectra%20as%20a%20function%20of%20the%20rotational%20and%20vibrational%20temperatures%20Delta%20v%3D-2.txt","description":"\u003Cp\u003ENMSSE  between two simulated spectra of the Delta v=-2 band sequence of the dicarbon Swan bands as a function of the rotational and vibrational temperature of the second spectrum. The first spectrum has a rotational and vibrational temperature of 4000\u2009K. Solely on the basis of the typical experimental signal-to-noise ratio a NMSSE of around 2.5 x 10^-7 is expected.\u003C\/p\u003E\n","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure C4d_NMSSE between two simulated spectra as a function of the rotational and vibrational temperatures Delta v=-2","mimetype":"text\/plain","size":"1.16 MB","created":"Tue, 06\/10\/2025 - 10:00","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"},{"id":"4c2e5e61-3a36-4923-9a88-cb4042f17c8d","revision_id":"","url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/Figure%20C5_Boltzmann%20plot.txt","description":"\u003Cp\u003EBoltzmann plot for an emission spectrum determined using Abel inversion from the space resolved spectra. The linear fit of the measured values corresponds to a rotational temperature of (3800\u2009\u00b1\u2009170) K.\u003C\/p\u003E\n","format":"txt","state":"Active","revision_timestamp":"Tue, 06\/10\/2025 - 10:04","name":"Figure C5_Boltzmann plot","mimetype":"text\/plain","size":"474 bytes","created":"Tue, 06\/10\/2025 - 10:02","resource_group_id":"ec8154f9-454d-4b85-895c-f5e010310847","last_modified":"Date changed  Tue, 06\/10\/2025 - 10:04"}],"groups":[{"description":"\u003Cp\u003EThe group \u0022Experimental Physics II - Reactive Plasmas\u0022 at the faculty of physics and astronomy at Ruhr University Bochum.\u003C\/p\u003E\n","id":"ec8154f9-454d-4b85-895c-f5e010310847","image_display_url":"https:\/\/rdpcidat.rub.de\/sites\/default\/files\/rublogoweiss_0.png","title":"EP2","name":"group\/ep2"}]}]}