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- ASTRONOMY and ASTROPHYSICS Is the FIP Effect Present Inside Solar Photospheric Magnetic flux Tubes?
- What Determines the Relative Areas of Spots and Faculae on Sun-Like Stars?
- Arxiv:1705.07054V1 [Astro-Ph.SR] 19 May 2017 2 Ilaria Ermolli Et Al
- 1 Introduction
- The Solar Chromosphere: the Inner Frontier of the Heliospheric System
- Large-Scale Photospheric Motions Determined from Granule Tracking and Helioseismology from SDO/HMI Data Th
- Tutorial: the Magnetic Connection Between the Sun and the Heliosphere
- Heliophysics I
- Correlation Between Sunspot Number and Ca II K Emission Index
- Local Helioseismology: Three Dimensional Imaging of the Solar Interior
- Chromospheric Emission, Rotation and X-Ray Coronae of Late-Type Stars R
- Chromospheric Heating by Acoustic Waves Compared to Radiative
- Solar Magnetic Atmospheric Effects on Global Helioseismic Oscillations
- Diagnosing the Frequency of Energy Deposition in the Magnetically
- Heliophysics Data Environment Enhancements Abstracts of Selected Proposals (NNH17ZDA001N-HDEE)
- Propagation of Coronal Mass Ejections in the Inner Heliosphere
- Interplanetary Space Weather Alerts: Science Benefits
- Investigating the Response of Loop Plasma to Nanoflare Heating Using
- How Faculae and Network Relate to Sunspots, and the Implications for Solar and Stellar Brightness Variations
- SOLIS: Reconciling Disk-Integrated and Disk-Resolved Spectra from the Sun
- Characterististics of Plage Fragments with Photospheric Network Properties
- Interplanetary Space Weather & Climate: a New Paradigm
- Investigating Magnetic Fields in the Solar Chromosphere
- Analysis of Ca <Superscript>+ </Superscript> K Plage Area For
- Causes of Solar Activity
- The Solar Atmosphere
- Properties of Solar Plage from a Spatially Coupled Inversion of Hinode SP Data D
- Transient Horizontal Magnetic Fields in Solar Plage Regions
- Critical Science Plan for the Daniel K. Inouye Solar Telescope (DKIST)
- Big Bear Solar Observatory
- A Century of Solar Ca II Measurements and Their Implication for Solar UV Driving of Climate
- Energetics of Magnetic Transients in a Solar Active Region Plage L
- Facular Structures on Cool Stars
- Historical Space Weather Forecasts and Synoptic Drawings Now
- HARPS-N Solar Rvs Are Dominated by Large, Bright Magnetic Regions
- Arxiv:2102.04864V1 [Astro-Ph.SR] 9 Feb 2021 1 Department of Physics, DSB Campus, Kumaun University, Nainital 263 002, India
- Solar Ca Ii K Plage Regions As Proxies for Magnetic Fields of Solar Like Stars
- A Model for the Formation of the Active Region Corona Driven by Magnetic flux Emergence? F
- A Century of Solar Ca II Measurements and Their Implication for Solar UV Driving of Climate
- Sanjiv K. Tiwari1,2*, Julia K. Thalmann3, Navdeep K. Panesar4, Ronald L