Standard

Solar irradiance observations with PREMOS filter radiometers on the PICARD mission : In-flight performance and data release. / Cessateur, G.; Schmutz, W.; Wehrli, C.; Groebner, J.; Haberreiter, M.; Kretzschmar, M.; Rozanov, E.; Schoell, M.; Shapiro, A.; Thuillier, G.; Finsterle, W.; Fox, N.; Hochedez, J. -F.; Koller, S.; Meftah, M.; Meindl, P.; Nyeki, S.; Pfiffner, D.; Roth, H.; Rouze, M.; Spescha, M.; Tagirov, R.; Wyss, J. -U.

в: ASTRONOMY & ASTROPHYSICS, Том 588, 126, 04.2016.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Cessateur, G, Schmutz, W, Wehrli, C, Groebner, J, Haberreiter, M, Kretzschmar, M, Rozanov, E, Schoell, M, Shapiro, A, Thuillier, G, Finsterle, W, Fox, N, Hochedez, J-F, Koller, S, Meftah, M, Meindl, P, Nyeki, S, Pfiffner, D, Roth, H, Rouze, M, Spescha, M, Tagirov, R & Wyss, J-U 2016, 'Solar irradiance observations with PREMOS filter radiometers on the PICARD mission: In-flight performance and data release', ASTRONOMY & ASTROPHYSICS, Том. 588, 126. https://doi.org/10.1051/0004-6361/201527577

APA

Cessateur, G., Schmutz, W., Wehrli, C., Groebner, J., Haberreiter, M., Kretzschmar, M., Rozanov, E., Schoell, M., Shapiro, A., Thuillier, G., Finsterle, W., Fox, N., Hochedez, J. -F., Koller, S., Meftah, M., Meindl, P., Nyeki, S., Pfiffner, D., Roth, H., ... Wyss, J. -U. (2016). Solar irradiance observations with PREMOS filter radiometers on the PICARD mission: In-flight performance and data release. ASTRONOMY & ASTROPHYSICS, 588, [126]. https://doi.org/10.1051/0004-6361/201527577

Vancouver

Cessateur G, Schmutz W, Wehrli C, Groebner J, Haberreiter M, Kretzschmar M и пр. Solar irradiance observations with PREMOS filter radiometers on the PICARD mission: In-flight performance and data release. ASTRONOMY & ASTROPHYSICS. 2016 Апр.;588. 126. https://doi.org/10.1051/0004-6361/201527577

Author

Cessateur, G. ; Schmutz, W. ; Wehrli, C. ; Groebner, J. ; Haberreiter, M. ; Kretzschmar, M. ; Rozanov, E. ; Schoell, M. ; Shapiro, A. ; Thuillier, G. ; Finsterle, W. ; Fox, N. ; Hochedez, J. -F. ; Koller, S. ; Meftah, M. ; Meindl, P. ; Nyeki, S. ; Pfiffner, D. ; Roth, H. ; Rouze, M. ; Spescha, M. ; Tagirov, R. ; Wyss, J. -U. / Solar irradiance observations with PREMOS filter radiometers on the PICARD mission : In-flight performance and data release. в: ASTRONOMY & ASTROPHYSICS. 2016 ; Том 588.

BibTeX

@article{63f3df3c29b549fc925961feb445baa8,
title = "Solar irradiance observations with PREMOS filter radiometers on the PICARD mission: In-flight performance and data release",
abstract = "Context. The PREcision Monitoring Sensor (PREMOS) is a solar radiometer on board the French PICARD mission that was launched in June 2010 and decommissioned in April 2014.Aims. The PREMOS radiometer obtains solar irradiance measurements in specific spectral windows in the UV, visible, and near-infrared. In this paper, the PREMOS data and calibration methods are presented.Methods. Using back-up channels, the degradation can theoretically be assessed to correct operational channels. However, a strong degradation within all PREMOS channels requires the application of additional methods, namely using back-up channels and assessing the degradation via a proxy-based model.Results. The corrected Level 3 PREMOS data are then used in different contexts in order to be validated. First, the signature of the p-mode are retrieved from the PREMOS data. The Venus transit allows us to empirically determine the intrinsic noise level within the PREMOS high cadence data for the visible and near-infrared channels. We then compare the PREMOS data directly to other data sets, namely from the SOLar-STellar Irradiance Comparison Experiment (SOLSTICE) and the Solar Irradiance Monitor (SIM) instruments on board the SOlar Radiation and Climate Experiment (SORCE) spacecraft. Regarding the UV channels, we found an excellent correlation over the lifetime of the PREMOS mission. The ratio between SORCE and PREMOS observations is always less than 1%. Regarding the SSI measurements in the visible and near-infrared, a comparison of short-term variations (i. e. 27-day modulation) shows a rather good correlation by taking into consideration the intrinsic noise within both SIM and PREMOS observations.",
keywords = "Sun: activity, instrumentation: photometers, Sun: UV radiation, solar-terrestrial relations, VARIABILITY, MODEL, LYRA, SUN, ULTRAVIOLET, FLARES, EUV",
author = "G. Cessateur and W. Schmutz and C. Wehrli and J. Groebner and M. Haberreiter and M. Kretzschmar and E. Rozanov and M. Schoell and A. Shapiro and G. Thuillier and W. Finsterle and N. Fox and Hochedez, {J. -F.} and S. Koller and M. Meftah and P. Meindl and S. Nyeki and D. Pfiffner and H. Roth and M. Rouze and M. Spescha and R. Tagirov and Wyss, {J. -U.}",
year = "2016",
month = apr,
doi = "10.1051/0004-6361/201527577",
language = "Английский",
volume = "588",
journal = "ASTRONOMY & ASTROPHYSICS",
issn = "0004-6361",
publisher = "EDP Sciences",

}

RIS

TY - JOUR

T1 - Solar irradiance observations with PREMOS filter radiometers on the PICARD mission

T2 - In-flight performance and data release

AU - Cessateur, G.

AU - Schmutz, W.

AU - Wehrli, C.

AU - Groebner, J.

AU - Haberreiter, M.

AU - Kretzschmar, M.

AU - Rozanov, E.

AU - Schoell, M.

AU - Shapiro, A.

AU - Thuillier, G.

AU - Finsterle, W.

AU - Fox, N.

AU - Hochedez, J. -F.

AU - Koller, S.

AU - Meftah, M.

AU - Meindl, P.

AU - Nyeki, S.

AU - Pfiffner, D.

AU - Roth, H.

AU - Rouze, M.

AU - Spescha, M.

AU - Tagirov, R.

AU - Wyss, J. -U.

PY - 2016/4

Y1 - 2016/4

N2 - Context. The PREcision Monitoring Sensor (PREMOS) is a solar radiometer on board the French PICARD mission that was launched in June 2010 and decommissioned in April 2014.Aims. The PREMOS radiometer obtains solar irradiance measurements in specific spectral windows in the UV, visible, and near-infrared. In this paper, the PREMOS data and calibration methods are presented.Methods. Using back-up channels, the degradation can theoretically be assessed to correct operational channels. However, a strong degradation within all PREMOS channels requires the application of additional methods, namely using back-up channels and assessing the degradation via a proxy-based model.Results. The corrected Level 3 PREMOS data are then used in different contexts in order to be validated. First, the signature of the p-mode are retrieved from the PREMOS data. The Venus transit allows us to empirically determine the intrinsic noise level within the PREMOS high cadence data for the visible and near-infrared channels. We then compare the PREMOS data directly to other data sets, namely from the SOLar-STellar Irradiance Comparison Experiment (SOLSTICE) and the Solar Irradiance Monitor (SIM) instruments on board the SOlar Radiation and Climate Experiment (SORCE) spacecraft. Regarding the UV channels, we found an excellent correlation over the lifetime of the PREMOS mission. The ratio between SORCE and PREMOS observations is always less than 1%. Regarding the SSI measurements in the visible and near-infrared, a comparison of short-term variations (i. e. 27-day modulation) shows a rather good correlation by taking into consideration the intrinsic noise within both SIM and PREMOS observations.

AB - Context. The PREcision Monitoring Sensor (PREMOS) is a solar radiometer on board the French PICARD mission that was launched in June 2010 and decommissioned in April 2014.Aims. The PREMOS radiometer obtains solar irradiance measurements in specific spectral windows in the UV, visible, and near-infrared. In this paper, the PREMOS data and calibration methods are presented.Methods. Using back-up channels, the degradation can theoretically be assessed to correct operational channels. However, a strong degradation within all PREMOS channels requires the application of additional methods, namely using back-up channels and assessing the degradation via a proxy-based model.Results. The corrected Level 3 PREMOS data are then used in different contexts in order to be validated. First, the signature of the p-mode are retrieved from the PREMOS data. The Venus transit allows us to empirically determine the intrinsic noise level within the PREMOS high cadence data for the visible and near-infrared channels. We then compare the PREMOS data directly to other data sets, namely from the SOLar-STellar Irradiance Comparison Experiment (SOLSTICE) and the Solar Irradiance Monitor (SIM) instruments on board the SOlar Radiation and Climate Experiment (SORCE) spacecraft. Regarding the UV channels, we found an excellent correlation over the lifetime of the PREMOS mission. The ratio between SORCE and PREMOS observations is always less than 1%. Regarding the SSI measurements in the visible and near-infrared, a comparison of short-term variations (i. e. 27-day modulation) shows a rather good correlation by taking into consideration the intrinsic noise within both SIM and PREMOS observations.

KW - Sun: activity

KW - instrumentation: photometers

KW - Sun: UV radiation

KW - solar-terrestrial relations

KW - VARIABILITY

KW - MODEL

KW - LYRA

KW - SUN

KW - ULTRAVIOLET

KW - FLARES

KW - EUV

U2 - 10.1051/0004-6361/201527577

DO - 10.1051/0004-6361/201527577

M3 - статья

VL - 588

JO - ASTRONOMY & ASTROPHYSICS

JF - ASTRONOMY & ASTROPHYSICS

SN - 0004-6361

M1 - 126

ER -

ID: 105535956