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Detection of Solar Rotational Variability in the Large Yield RAdiometer (LYRA) 190-222 nm Spectral Band. / Dominique, M.; Dammasch, I. E.; Wehrli, C.; Rozanov, E.; Schmutz, W.

In: Solar Physics, Vol. 286, No. 1, 08.2013, p. 289-301.

Research output: Contribution to journal › Article › peer-review

Harvard

Dominique, M, Dammasch, IE, Wehrli, C, Rozanov, E & Schmutz, W 2013, 'Detection of Solar Rotational Variability in the Large Yield RAdiometer (LYRA) 190-222 nm Spectral Band', Solar Physics, vol. 286, no. 1, pp. 289-301. https://doi.org/10.1007/s11207-012-0029-2

APA

Dominique, M., Dammasch, I. E., Wehrli, C., Rozanov, E., & Schmutz, W. (2013). Detection of Solar Rotational Variability in the Large Yield RAdiometer (LYRA) 190-222 nm Spectral Band. Solar Physics, 286(1), 289-301. https://doi.org/10.1007/s11207-012-0029-2

Vancouver

Dominique M, Dammasch IE, Wehrli C, Rozanov E, Schmutz W. Detection of Solar Rotational Variability in the Large Yield RAdiometer (LYRA) 190-222 nm Spectral Band. Solar Physics. 2013 Aug;286(1):289-301. https://doi.org/10.1007/s11207-012-0029-2

Author

Dominique, M. ; Dammasch, I. E. ; Wehrli, C. ; Rozanov, E. ; Schmutz, W. / Detection of Solar Rotational Variability in the Large Yield RAdiometer (LYRA) 190-222 nm Spectral Band. In: Solar Physics. 2013 ; Vol. 286, No. 1. pp. 289-301.

BibTeX

@article{8fa71f5d1aec44ef9b3862888f4dcd9d,
title = "Detection of Solar Rotational Variability in the Large Yield RAdiometer (LYRA) 190-222 nm Spectral Band",
abstract = "We analyze the variability of the spectral solar irradiance during the period from 7 January 2010 until 20 January 2010 as measured by the Herzberg channel (190 -aEuro parts per thousand 222 nm) of the Large Yield RAdiometer (LYRA) onboard PROBA2. In this period of time, observations by the LYRA nominal unit experienced degradation and the signal produced by the Herzberg channel frequently jumped from one level to another. Both factors significantly complicate the analysis. We present the algorithm that allowed us to extract the solar variability from the LYRA data and compare the results with SORCE/SOLSTICE measurements and with modeling based on the Code for the Solar Irradiance (COSI).",
keywords = "IRRADIANCE VARIATIONS, MODELS",
author = "M. Dominique and Dammasch, {I. E.} and C. Wehrli and E. Rozanov and W. Schmutz",
year = "2013",
month = aug,
doi = "10.1007/s11207-012-0029-2",
language = "Английский",
volume = "286",
pages = "289--301",
journal = "Solar Physics",
issn = "0038-0938",
publisher = "Springer Nature",
number = "1",

}

RIS

TY - JOUR

T1 - Detection of Solar Rotational Variability in the Large Yield RAdiometer (LYRA) 190-222 nm Spectral Band

AU - Dominique, M.

AU - Dammasch, I. E.

AU - Wehrli, C.

AU - Rozanov, E.

AU - Schmutz, W.

PY - 2013/8

Y1 - 2013/8

N2 - We analyze the variability of the spectral solar irradiance during the period from 7 January 2010 until 20 January 2010 as measured by the Herzberg channel (190 -aEuro parts per thousand 222 nm) of the Large Yield RAdiometer (LYRA) onboard PROBA2. In this period of time, observations by the LYRA nominal unit experienced degradation and the signal produced by the Herzberg channel frequently jumped from one level to another. Both factors significantly complicate the analysis. We present the algorithm that allowed us to extract the solar variability from the LYRA data and compare the results with SORCE/SOLSTICE measurements and with modeling based on the Code for the Solar Irradiance (COSI).

AB - We analyze the variability of the spectral solar irradiance during the period from 7 January 2010 until 20 January 2010 as measured by the Herzberg channel (190 -aEuro parts per thousand 222 nm) of the Large Yield RAdiometer (LYRA) onboard PROBA2. In this period of time, observations by the LYRA nominal unit experienced degradation and the signal produced by the Herzberg channel frequently jumped from one level to another. Both factors significantly complicate the analysis. We present the algorithm that allowed us to extract the solar variability from the LYRA data and compare the results with SORCE/SOLSTICE measurements and with modeling based on the Code for the Solar Irradiance (COSI).

KW - IRRADIANCE VARIATIONS

KW - MODELS

U2 - 10.1007/s11207-012-0029-2

DO - 10.1007/s11207-012-0029-2

M3 - статья

VL - 286

SP - 289

EP - 301

JO - Solar Physics

JF - Solar Physics

SN - 0038-0938

IS - 1

ER -

ID: 105538006