Observing Interstellar Neutral Helium from the Ground

Details Observing Interstellar Neutral Helium from the Ground Observing Interstellar Neutral Helium from the Ground

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agufmsh14a1698m&link_type=abstract

American Geophysical Union, Fall Meeting 2007, abstract #SH14A-1698

Physics

2126 Heliosphere/Interstellar Medium Interactions, 2129 Interplanetary Dust, 7509 Corona, 7599 General Or Miscellaneous, 7837 Neutral Particles (2151)

Scientific paper

Cool neutral Helium is now being observed near the Sun. Routinely from sensitive IR spectropolarimetry data using SOLARC at Haleakala and from eclipses, observations reveal scattered photospheric light at 1083nm from He I far above the solar limb. Here we report on observations of this transient coronal constituent that help to understand whether this comes from the coronal "inner source" or from the interstellar Helium wind.

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