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Critical Science Plan for the Daniel K. Inouye Solar Telescope (DKIST)
DOI: 10.1007/s11207-021-01789-2 Bibcode: 2021SoPh..296...70R

Andretta, Vincenzo; Ayres, Thomas R.; Liu, Wei +87 more

The National Science Foundation's Daniel K. Inouye Solar Telescope (DKIST) will revolutionize our ability to measure, understand, and model the basic physical processes that control the structure and dynamics of the Sun and its atmosphere. The first-light DKIST images, released publicly on 29 January 2020, only hint at the extraordinary capabiliti…

2021 Solar Physics
IRIS 82
A New View of the Solar Interface Region from the Interface Region Imaging Spectrograph (IRIS)
DOI: 10.1007/s11207-021-01826-0 Bibcode: 2021SoPh..296...84D

Reeves, Katharine K.; Polito, Vanessa; Liu, Wei +11 more

The Interface Region Imaging Spectrograph (IRIS) has been obtaining near- and far-ultraviolet images and spectra of the solar atmosphere since July 2013. IRIS is the highest resolution observatory to provide seamless coverage of spectra and images from the photosphere into the low corona. The unique combination of near- and far-ultraviolet spectra…

2021 Solar Physics
Hinode IRIS 58
Upflows in the Upper Solar Atmosphere
DOI: 10.1007/s11207-021-01792-7 Bibcode: 2021SoPh..296...47T

Tian, Hui; Brooks, David H.; Baker, Deborah +2 more

Spectroscopic observations at extreme- and far-ultraviolet wavelengths have revealed systematic upflows in the solar transition region and corona. These upflows are best seen in the network structures of the quiet Sun and coronal holes, boundaries of active regions, and dimming regions associated with coronal mass ejections. They have been intensi…

2021 Solar Physics
Hinode IRIS SOHO SolarOrbiter 44
Probabilistic Drag-Based Ensemble Model (DBEM) Evaluation for Heliospheric Propagation of CMEs
DOI: 10.1007/s11207-021-01859-5 Bibcode: 2021SoPh..296..114C

Veronig, Astrid M.; Dumbović, Mateja; Temmer, Manuela +4 more

The Drag-based Model (DBM) is a 2D analytical model for heliospheric propagation of Coronal Mass Ejections (CMEs) in ecliptic plane predicting the CME arrival time and speed at Earth or any other given target in the solar system. It is based on the equation of motion and depends on initial CME parameters, background solar wind speed, w and the dra…

2021 Solar Physics
SOHO 29
Assessing the Predictability of Solar Energetic Particles with the Use of Machine Learning Techniques
DOI: 10.1007/s11207-021-01837-x Bibcode: 2021SoPh..296..107L

Lavasa, E.; Giannopoulos, G.; Papaioannou, A. +5 more

A consistent approach for the inherently imbalanced problem of solar energetic particle (SEP) events binary prediction is being presented. This is based on solar flare and coronal mass ejection (CME) data and combinations of both thereof. We exploit several machine learning (ML) and conventional statistics techniques to predict SEPs. The methods u…

2021 Solar Physics
SOHO 28
Role of Compressive Viscosity and Thermal Conductivity on the Damping of Slow Waves in Coronal Loops with and Without Heating-Cooling Imbalance
DOI: 10.1007/s11207-021-01764-x Bibcode: 2021SoPh..296...20P

Srivastava, A. K.; Wang, T. J.; Prasad, Abhinav

In the present article, we derive a new dispersion relation for slow magnetoacoustic waves invoking the effect of thermal conductivity, compressive viscosity, radiation, and an unknown heating term along with the consideration of heating-cooling imbalance from linearized MHD equations. We solve the general dispersion relation to understand the rol…

2021 Solar Physics
SOHO 26
Measurements of Solar Differential Rotation Using the Century Long Kodaikanal Sunspot Data
DOI: 10.1007/s11207-021-01767-8 Bibcode: 2021SoPh..296...25J

Chatterjee, Subhamoy; Banerjee, Dipankar; Jha, Bibhuti Kumar +2 more

The rotational profile of the Sun is considered to be one of the key inputs in a solar dynamo model. Hence, precise and long-term measurements of this quantity is important for our understanding of solar magnetism and its variability. In this study, we use the newly digitised, white-light sunspot data (1923 - 2011) from Kodaikanal Solar Observator…

2021 Solar Physics
SOHO 25
CME-Driven and Flare-Ignited Fast Magnetosonic Waves Detected in a Solar Eruption
DOI: 10.1007/s11207-021-01913-2 Bibcode: 2021SoPh..296..169Z

Shen, Yuandeng; Zhou, Chengrui; Zhou, Xinping +4 more

We present Solar Dynamics Observatory/Atmospheric Imaging Assembly (SDO/AIA) observation of three types of fast-mode, propagating, magnetosonic waves in a GOES C3.0 flare on 23 April 2013, which was accompanied by a prominence eruption and a broad coronal mass ejection (CME). During the fast-rising phase of the prominence, a large-scale, dome-shap…

2021 Solar Physics
SOHO 24
Science Highlights and Final Updates from 17 Years of Total Solar Irradiance Measurements from the SOlar Radiation and Climate Experiment/Total Irradiance Monitor (SORCE/TIM)
DOI: 10.1007/s11207-021-01853-x Bibcode: 2021SoPh..296..133K

Kopp, Greg

The final version (V.19) of the total solar irradiance data from the SOlar Radiation and Climate Experiment (SORCE) Total Irradiance Monitor has been released. This version includes all calibrations updated to the end of the mission and provides irradiance data from 25 February 2003 through 25 February 2020. These final calibrations are presented …

2021 Solar Physics
SOHO 24
Empirical Model of 10 - 130 MeV Solar Energetic Particle Spectra at 1 AU Based on Coronal Mass Ejection Speed and Direction
DOI: 10.1007/s11207-021-01779-4 Bibcode: 2021SoPh..296...36B

Richardson, Ian G.; Bruno, Alessandro

We present a new empirical model to predict solar energetic particle (SEP) event-integrated and peak intensity spectra between 10 and 130 MeV at 1 AU, based on multi-point spacecraft measurements from the Solar TErrestrial RElations Observatory (STEREO), the Geostationary Operational Environmental Satellites (GOES), and the Payload for Antimatter …

2021 Solar Physics
SOHO 22