CLASP2: The Chromospheric LAyer Spectro-Polarimeter
Informazioni aggiuntive
Autori
Rachmeler L.,
McKenzie D. E.,
Ishikawa R.,
Bueno J. T.,
Auchère F.,
Kobayashi K.,
Winebarger A.,
Bethge C.,
Kano R.,
Kubo M.,
Song D.,
Narukage N.,
Ishikawa S.,
Pontieu B. D.,
Carlsson M.,
Yoshida M.,
Belluzzi L.,
Stepan J.,
Alemná T. d. P.,
Alsina Ballester E.,
Ramos A. A.
Tipo
Contributo in atti di convegno
Anno
2017
Lingua
Inglese
Sommario
We present the instrument, science case, and timeline of the CLASP2sounding rocket mission. The successful CLASP (Chromospheric Lyman-Alpha Spectro-Polarimeter) sounding rocket flight in 2015 resulted in the first-ever linear polarization measurements of solar hydrogen Lyman-alpha line, which is sensitive to the Hanle effect and can be used to constrain the magnetic field and geometric complexity of the upper chromosphere. Ly-alpha is one of several upper chromospheric lines that contain magnetic information. In the spring of 2019, we will re-fly the modified CLASP telescope to measure the full Stokes profile of Mg II h amp k near 280 nm. This set of lines is sensitive to the upper chromospheric magnetic field via both the Hanle and the Zeeman effects.
Parole chiave
irsol-conference-proceedings
Titolo atti di convegno
AAS/Solar Physics Division Meeting
Collana
AAS/Solar Physics Division Meeting
Pagine (o numero dell’articolo)
110.10
