The Relationship Between X-Ray Radiance and Magnetic Flux

By A. Pevtsov, G. Fisher, L. Acton, D. Longcope, C. Johns–Krull, C. Kankelborg, T. Metcalf. 2003

243 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/11321a11ef56f89ccb36d154f2e416e582a00d29

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In Astronomy and Astrophysics

Citations in the corpus

MAGNETOHYDRODYNAMIC WAVES AND CORONAL HEATING: UNIFYING EMPIRICAL AND MHD TURBULENCE MODELS (2012, methodology): “Nevertheless, the estimate is very close to that which follows from Pevtsov et al. (2003); Abbett (2007); Downs et al. (2010).”
The Magnetic Connection between the Convection Zone and Corona in the Quiet Sun (2007, methodology): “However, there is strong observational evidence that argues for a universal relationship between unsigned magnetic flux and the power dissipated through a coronal heating mechanism (Fisher et al. 1998; Pevtsov et al. 2003; Lundquist et al. 2007b;Warren &Winebarger 2006).”
The Sun in Time: Activity and Environment (2007, background): “The average surface magnetic fields of CTTS also exceed a prediction from X-rays, based on a correlation between X-ray luminosity and photospheric magnetic flux valid for MS stars and the Sun (Pevtsov et al., 2003).”
Stellar winds on the main-sequence - II. The evolution of rotation and winds (2015, unknown): “15B from Pevtsov et al. (2003) with the relation between RX (where RX = LX/Lbol) and Rossby number of RX ∝ P−2.18rot from Wright et al. (2011) would imply for a given stellar mass that fB ∝ P−1.9rot , though using the steeper relation of RX ∝ P−2.7rot from Wright et al. (2011) would imply that fB ∝…”
The Magnetic Fields of Classical T Tauri Stars (2007, methodology): “Pevtsov et al. (2003) study the relationship betweenmagnetic flux and X-ray luminosity on the Sun and cool stars, generally finding excellent correlation between these two quantities ranging over almost 11 orders of magnitude in each quantity.”
Stellar magnetism: empirical trends with age and rotation (2014, background): “…From ZB Reference 〈|BV |〉 ∝ P−1.32±0.14rot 〈|BI |〉 ∝ P −1.7 rot Saar (1996) 〈|BV |〉 ∝ Ro−1.38±0.14 〈|BI |〉 ∝ Ro−1.2 Saar (2001) L (all) X ∝ Φ 0.913±0.054 V L (all) X ∝ Φ 1.13 I Pevtsov et al. (2003) L (dwarfs) X ∝ Φ 1.80±0.20 V L (dwarfs) X ∝ Φ 0.98±0.19 I Pevtsov et al. (2003) LX/Lbol ∝ 〈|BV…”
Flux tube texture of the solar wind: Strands of the magnetic carpet at 1 AU?: FLUX TUBE TEXTURE OF SOLAR WIND (2008, background): “…et al., 1999; Priest et al., 2002; Klimchuk, 2006], about the magnetic carpet [e.g., Parnell, 2001; Haganaar et al., 1997; Schrijver and Title, 2003; Wang and Sheeley, 2004], and about stellar winds in general [Landstreet, 1992; Schmelz, 2003; Pevtsov et al., 2003; Gudel, 2004; Holzwarth, 2005].”
Interplanetary flux rope ejected from an X-ray bright point. The smallest magnetic cloud source-region ever observed (2005, background): “Pevtsov et al. (2003) extended this result to a broad range of structures on the Sun (quiet Sun, X-ray bright points, active regions, and integrated solar disc) and to active stars (dwarf and pre-main-sequence).”
On the Correlation between the Magnetic Activity Levels, Metallicities, and Radii of Low-Mass Stars (2007, background): “Many of the stars in the sample havemetallicity estimates and measured X-ray fluxes, a good indicator of magnetic activity (Pevtsov et al. 2003).”
TESTING A PREDICTIVE THEORETICAL MODEL FOR THE MASS LOSS RATES OF COOL STARS (2011, result): “Its agreement with the behavior off∗ shown above is also consistent with existing empirical correlations between X-rays and magnetic activity (Pevtsov et al. 2003).”
Can Superflares Occur on Our Sun (2012, background): “CVn) are magnetically very active (e.g., Pallavicini et al. 1981; Pevtsov et al. 2003) and show many superflares (e.g., Shibata & Yokoyama 2002).”
MULTISPECTRAL EMISSION OF THE SUN DURING THE FIRST WHOLE SUN MONTH: MAGNETOHYDRODYNAMIC SIMULATIONS (2008, background): “Pevtsov et al. (2003) concluded that there is a universal linear correlation between magnetic flux and X-ray radiance.”
Statistical properties of superflares on solar-type stars based on 1-min cadence data (2015, background): “The empirical relation between the X-ray luminosity and the magnetic flux of the star (Pevtsov et al. 2003) suggests that themagnetic flux of KIC 7093428”