Search NASA⌕ Search
Home/Archive/NASA NTRS

NASA NTRS · 20205004163

The Chromospheric LAyer SpectroPolarimeter (CLASP2) Mission: Introduction

David E McKenzie·Ryohko Ishikawa·Ryouhei Kano·Laurel Rachmeler·Javier Trujillo Bueno·Ken Kobayashi·Donguk Song·Masaki Yoshida·Frederic Auchere·Joten Okamoto·Tanausu del Pino Aleman
View original source ↗Export metadata ↓

Abstract

The source did not provide an abstract. Follow the original record for more information.

Explore related subjects

chromospheresounding rockets

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

David E McKenzie, Ryohko Ishikawa, Ryouhei Kano, Laurel Rachmeler, Javier Trujillo Bueno, Ken Kobayashi, Donguk Song, Masaki Yoshida, Frederic Auchere, Joten Okamoto, Tanausu del Pino Aleman. The Chromospheric LAyer SpectroPolarimeter (CLASP2) Mission: Introduction. https://ntrs.nasa.gov/citations/20205004163

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related reports

NASA NTRSDate not supplied

Even Small Events Involve the Entire Solar Atmosphere

The connection between the photosphere, chromosphere, and corona is essential for understanding the energy flows throughout the solar atmosphere. Here we discuss and analyze observations centered on a bipolar region of enhanced-network magnetic flux near disk center on SOL2017-03-17T14:00-17:00. The comprehensive data set comprises observations from SDO: HMI, AIA; Hinode: SOT, XRT; DST: IBIS, FIRS; ALMA; and IRIS; thus providing a variety of plasma diagnostics spanning the photosphere to the corona. Numerous transient brightenings were observed across the data set, and here we highlight transient brightenings within a set of thin filamentary features. One interesting event shows initial heating in the cooler (ALMA, 7000 K) before showing in the hotter (XRT, 3 MK) data series. These brightenings showcase how even small events involve large ranges of the solar atmosphere.

chromosphere↗