Solar Irradiance Reference Spectra (SIRS) for the 2008 Whole Heliosphere Interval (WHI)

By T. Woods, P. Chamberlin, J. Harder, R. Hock, M. Snow, F. Eparvier, J. Fontenla, W. McClintock, E. Richard. 2008

187 citations recorded by the source corpus.

Subfields: Artificial Intelligence, Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/1e6eed8750c9ef221160974f12d04688cceb7026

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Artificial Intelligence

1. S. Solanki
2. N. Krivova
3. J. Haigh
4. C. Willmer
5. K. L. Yeo
6. Karl-Heinz Glassmeier
7. J. Fontenla
8. J. Harder

In Astronomy and Astrophysics

1. N. Krivova
2. S. Solanki
3. J. Haigh
4. Liying Qian
5. T. Woods
6. Karl-Heinz Glassmeier
7. K. L. Yeo
8. S. Solomon

In Atmospheric Science

1. S. Solanki
2. N. Krivova
3. C. Willmer
4. Liying Qian
5. T. Woods
6. S. Solomon
7. J. Haigh
8. R. Viereck

Citations in the corpus

• The Absolute Magnitude of the Sun in Several Filters (2018, methodology): “Figure 2 shows the ratios between this composite spectrum with other determinations in the literature – Rieke et al. (2008); Thuillier et al. (2004); Woods et al. (2009).”
• SEMIEMPIRICAL MODELS OF THE SOLAR ATMOSPHERE. III. SET OF NON-LTE MODELS FOR FAR-ULTRAVIOLET/EXTREME-ULTRAVIOLET IRRADIANCE COMPUTATION (2009, methodology): “Figure 10 shows the solar irradiance for a quiet-Sun day (2008 April 14) computed by SRPM from the present models and the spectra observed by the SORCE/SOLSTICE instrument (Woods et al. 2009) and the EVE instrument on a rocket flight (Chamberlin et al. 2008).”
• Causes of low thermospheric density during the 2007–2009 solar minimum (2011, background): “There is some independent confirmation of these changes from other suborbital flights, and from TIMED/SEE [ Woods et al., 1998, 2005, 2009; Chamberlin et al., 2009], but the uncertainty estimates for these measurements are significant, as discussed by Solomon et al. [2010].”
• THE ULTRAVIOLET RADIATION ENVIRONMENT AROUND M DWARF EXOPLANET HOST STARS (2012, methodology): “The UV (FUV + NUV) spectra of solar-type stars have been studied extensively, both observationally and theoretically (e.g., Woods et al. 2009; Fontenla et al. 2011; Linsky et al. 2012c).”
• THE MUSCLES TREASURY SURVEY. I. MOTIVATION AND OVERVIEW (2016, unknown): “However, obtaining a complete EUV spectrum of any cool star other than the Sun is currently impossible owing to attenuation by the ISM.”
• Anomalously low solar extreme‐ultraviolet irradiance and thermospheric density during solar minimum (2010, background): “Also shown on this plot are measurements during the two solar minima by different instruments integrated over the same wavelength band, including two rocket flights [ Woods et al., 1998, 2009; Chamberlin et al., 2009], and the average of SEE daily measurements during 2008.”
• Reconstruction of total and spectral solar irradiance from 1974 to 2013 based on KPVT, SoHO/MDI and SDO/HMI observations (2014, methodology): “– 180 to 300 nm: We offset this segment of the reconstruction (wavelength element by wavelength element) to the Whole Heliospheric Interval (WHI) reference solar spectra (version 2, Woods et al. 2009).”
• Solar Irradiance Variability and Climate (2013, methodology): “More recent solar reference spectra were produced within the Whole Heliosphere Interval (WHI) international campaign during three relatively quiet periods in March–April 2008 (Woods et al. 2009).”