Solar EUV Experiment (SEE): Mission overview and first results

By T. Woods, F. Eparvier, S. Bailey, P. Chamberlin, J. Lean, G. Rottman, S. Solomon, W. Tobiska, D. Woodraska. 2005

487 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/811cc1c0faa65fd6771256a66f2d79101a2acaba

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In Astronomy and Astrophysics

1. N. Krivova
2. S. Solanki
3. T. Woods
4. Liying Qian
5. C. Fröhlich
6. P. Chamberlin
7. S. Solomon
8. J. Lean

In Atmospheric Science

1. S. Solanki
2. N. Krivova
3. P. Chamberlin
4. Liying Qian
5. T. Woods
6. S. Solomon
7. F. Eparvier
8. J. Lean

Citations in the corpus

• ATMOSPHERIC ESCAPE FROM HOT JUPITERS (2008, background): “For a UV flux near the Lyman edge that is ∼2–3 times larger, as obtains during solar maximum (Woods et al. 2005; Lean et al. 2003, and references therein), the mass loss rate is ∼2 × 1010 g s−1 (we have shown that at these fluxes, mass loss is energylimited and scales nearly linearly with UV flux).”
• Unexpected variability of Martian hydrogen escape (2014, methodology): “…we scale, and phase delay to Mars according to the procedures of Mitchell et al. [2001], or in the total solar spectral irradiance below 90 nm as measured by the Solar Extreme ultraviolet Explorer on NASA’s Thermosphere Ionosphere Mesosphere Energetics and Dynamics mission [ Woods et al. , 2005].”
• Anomalously low solar extreme‐ultraviolet irradiance and thermospheric density during solar minimum (2010, background): “…2010 L16103 1 of 5 Monitor (SEM) [Judge et al., 1998] on the Solar and Heliospheric Observatory (SOHO), the Solar EUV Experiment (SEE) [Woods et al., 2005] on the Thermosphere‐Ionosphere‐ Mesosphere Energetics and Dynamics (TIMED) satellite, and several sub‐orbital rocket flights…”
• Solar Irradiance Reference Spectra (SIRS) for the 2008 Whole Heliosphere Interval (WHI) (2008, methodology): “For TIMED SEE, the long-term degradation is derived from weekly calibrations with redundant channels and five underflight rocket calibrations made between 2002 and 2008 [Woods et al., 2005a].”
• Causes of low thermospheric density during the 2007–2009 solar minimum (2011, background): “Measurements of solar EUV levels are available from several space‐based experiments, including the Solar EUV Monitor (SEM) [Judge et al., 1998] on the Solar and Heliospheric Observatory (SOHO), the Solar EUV Experiment (SEE) [Woods et al., 2005] on the Thermosphere‐Ionosphere‐Mesosphere Energetics a”
• Negative ion chemistry in Titan's upper atmosphere (2008, methodology): “The solar flux used in the calculations is the measured flux by the TIMED/SEE instrument during the T40 flyby, scaled to Saturn’s location (Woods, 2008; Woods et al., 2005).”
• GLOBAL ENERGETICS OF THIRTY-EIGHT LARGE SOLAR ERUPTIVE EVENTS (2012, methodology): “It uses measurements in this wavelength range from the Solar EUV Experiment (SEE; Woods et al. 2005) on the Thermosphere Ionosphere Mesosphere Energetics and Dynamics (TIMED) satellite and the SOLar-STellar Irradiance Comparison Experiment (SOLSTICE; Rottman et al. 1993) on the Upper Atmosphere…”
• Solar extreme‐ultraviolet irradiance for general circulation models (2005, methodology): “[28] We have also used data from the SEE instrument on the NASA TIMED satellite [Woods et al., 1998b, 2005] to drive the TIE-GCM.”
• Extreme Ultraviolet Variability Experiment (EVE) on the Solar Dynamics Observatory (SDO): Overview of Science Objectives, Instrument Design, Data Products, and Model Developments (2010, methodology): “The current TIMED Solar EUV Experiment (SEE) measurements (Woods et al., 2005) have improved the absolute accuracy of the solar EUV spectral irradiances to about 20%, and the Figure 3 EVE instrument spectral ranges.”