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電子書籍・電子雑誌EPS : Earth, Planets and Space
Volume number67
Statistica...

Statistical properties of superflares on solar-type stars based on 1-min cadence data

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Statistical properties of superflares on solar-type stars based on 1-min cadence data

Call No. (NDL)
Z14-196
Bibliographic ID of National Diet Library
9483544
Persistent ID (NDL)
info:ndljp/pid/9483544
Material type
記事
Author
Hiroyuki Maeharaほか
Publisher
Springer science+business media
Publication date
2015-04-29
Material Format
Paper・Digital
Journal name
EPS : Earth, Planets and Space 67(59)
Publication Page
-
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We searched for superflares on solar-type stars using Kepler data with 1-min sampling in order to detect superflares with a short duration. We found 1...

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Digital

Material Type
記事
Author/Editor
Hiroyuki Maehara
Takuya Shibayama
Yuta Notsu
Publication, Distribution, etc.
Publication Date
2015-04-29
Publication Date (W3CDTF)
2015-04-29
Periodical title
EPS : Earth, Planets and Space
No. or year of volume/issue
67(59)
Volume
67(59)
ISSN (Periodical Title)
1880-5981
ISSN-L (Periodical Title)
1343-8832
Text Language Code
eng
Persistent ID (NDL)
info:ndljp/pid/9483544
Collection (Materials For Handicapped People:1)
Collection (particular)
国立国会図書館デジタルコレクション > 電子書籍・電子雑誌 > その他
Acquisition Basis
オンライン資料収集制度
Date Accepted (W3CDTF)
2015-08-17T20:47:01+09:00
Date Captured (W3CDTF)
2015-06-20
Format (IMT)
application/pdf
Access Restrictions
国立国会図書館内限定公開
Service for the Digitized Contents Transmission Service
図書館・個人送信対象外
Availability of remote photoduplication service
Periodical Title (Persistent ID (NDL))
info:ndljp/pid/9227920
Data Provider (Database)
国立国会図書館 : 国立国会図書館デジタルコレクション

Digital

Summary, etc.
We searched for superflares on solar-type stars using Kepler data with 1-min sampling in order to detect superflares with a short duration. We found 187 superflares on 23 solar-type stars whose bolometric energy ranges from the order of 10<sup>32</sup> to 10<sup>36</sup> erg. Some superflares show multiple peaks with the peak separation of the order of 100 to 1, 000 s which is comparable to the periods of quasi-periodic pulsations in solar and stellar flares. Using these new data combined with the results from the data with 30-min sampling, we found that the occurrence frequency (dN/dE) of superflares as a function of flare energy (E) shows the power-law distribution (dN/dE∞E <sup>-α</sup> ) with α∼-1.5 for 10<sup>33</sup><E<10<sup>36</sup> erg which is consistent with the previous results. The average occurrence rate of superflares with the energy of 10<sup>33</sup> erg which is equivalent to X100 solar flares is about once in 500 to 600 years. The upper limit of energy released by superflares is basically comparable to a fraction of the magnetic energy stored near starspots which is estimated from the photometry. We also found that the duration of superflares (τ) increases with the flare energy (E) as τ∞E <sup>0.39 ± 0.03</sup>. This can be explained if we assume the time scale of flares is determined by the Alfvén time.
Access Restrictions
インターネット公開
Rights (production)
© 2015 Maehara et al.; licensee Springer. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly credited.
Is Referenced By
Discovery of a long-duration superflare on a young solar-type star EK Draconis with nearly similar time evolution for Ha and white-light emissions
Historical Auroras in the 990s: Evidence of Great Magnetic Storms
High dispersion spectroscopy of solar-type superflare stars. III. Lithium abundances
Spectroscopic observations of active solar-analog stars with high X-ray luminosity, as a proxy of superflare stars
Fractal Reconnection in Solar and Stellar Environments
Low-latitude Aurorae during the Extreme Space Weather Events in 1859
Lifetimes and Emergence/Decay Rates of Star Spots on Solar-type Stars Estimated by Kepler Data in Comparison with Those of Sunspots
Do Kepler Superflare Stars Really Include Slowly Rotating Sun-like Stars?—Results Using APO 3.5 m Telescope Spectroscopic Observations and Gaia-DR2 Data
Probability Distribution Functions of Solar and Stellar Flares
Apache Point Observatory (APO)/SMARTS Flare Star Campaign Observations. I. Blue Wing Asymmetries in Chromospheric Lines during Mid-M-Dwarf Flares from Simultaneous Spectroscopic and Photometric Observation Data
Rising Near-ultraviolet Spectra in Stellar Megaflares
Statistical Studies of Solar White-light Flares and Comparisons with Superflares on Solar-type Stars
On the Size of the Flare Associated with the Solar Proton Event in 774 AD
Time-resolved spectroscopy and photometry of M dwarf flare star YZ Canis Minoris with OISTER and TESS: Blue asymmetry in the Hα line during the non-white light flare
Statistical Properties of Superflares on Solar-type Stars: Results Using All of the Kepler Primary Mission Data
Extreme solar events
Reconstructing the XUV Spectra of Active Sun-like Stars Using Solar Scaling Relations with Magnetic Flux
Effect of Time-varying X-Ray Emission from Stellar Flares on the Ionization of Protoplanetary Disks
The Characteristics of Solar X-Class Flares and CMEs: A Paradigm for Stellar Superflares and Eruptions?
Starspot activity and superflares on solar-type stars
MAGNETIC PROPERTIES OF SOLAR ACTIVE REGIONS THAT GOVERN LARGE SOLAR FLARES AND ERUPTIONS
The Celestial Sign in the Anglo-Saxon Chronicle in the 770s: Insights on Contemporary Solar Activity
{High dispersion spectroscopy of solar-type superflare stars with Subaru/HDS
Recurrent Large‐Scale Solar Proton Events Before the Onset of the Wolf Grand Solar Minimum
Supernovae and Single-Year Anomalies in the Atmospheric Radiocarbon Record
A great space weather event in February 1730
Modeling Hadronic Gamma-Ray Emissions from Solar Flares and Prospects for Detecting Nonthermal Signatures from Protostars
Temporal Variation of Flare Occurrence Rates via the Spot Evolution on the Sun and Solar-type Stars
Impact of Stellar Superflares on Planetary Habitability
South American auroral reports during the Carrington storm
References
Solar Flares: Magnetohydrodynamic Processes
A signature of cosmic-ray increase in ad 774–775 from tree rings in Japan
Superflares on Ordinary Solar‐Type Stars
<i>GALEX</i>high time-resolution ultraviolet observations of dMe flare events
<i>RHESSI</i>Microflare Statistics. I. Flare‐Finding and Frequency Distributions
Frequency distributions and correlations of solar X-ray flare parameters
INITIAL CHARACTERISTICS OF <i>KEPLER</i> SHORT CADENCE DATA
Superflares on solar-type stars
SUPERFLARES ON SOLAR-TYPE STARS OBSERVED WITH <i>KEPLER</i> . I. STATISTICAL PROPERTIES OF SUPERFLARES
High dispersion spectroscopy of solar-type superflare stars. I. Temperature, surface gravity, metallicity, and <i>v</i>sin <i>i</i>
The Dependence of Large Flare Occurrence on the Magnetic Structure of Sunspots
<i>Kepler</i>super-flare stars: what are they?
High dispersion spectroscopy of solar-type superflare stars. II. Stellar rotation, starspots, and chromospheric activities
Time Variability of the “Quiet” Sun Observed with<i>TRACE</i>. II. Physical Parameters, Temperature Evolution, and Energetics of Extreme‐Ultraviolet Nanoflares
Temporal aspects and frequency distributions of solar soft X-ray flares
Another rapid event in the carbon-14 content of tree rings
SUPERFLARES ON SOLAR-TYPE STARS OBSERVED WITH<i>KEPLER</i>II. PHOTOMETRIC VARIABILITY OF SUPERFLARE-GENERATING STARS: A SIGNATURE OF STELLAR ROTATION AND STARSPOTS
SUPERFLARE OCCURRENCE AND ENERGIES ON G-, K-, AND M-TYPE DWARFS
Can Superflares Occur on Our Sun?
High-Dispersion Spectroscopy of the Superflare Star KIC 6934317
Two sun-like superflare stars rotating as slow as the Sun
Flashes from normal stars
THE DECAYING LONG-PERIOD OSCILLATION OF A STELLAR MEGAFLARE
Quasi-Periodic Pulsations in Solar Flares
Estimating the frequency of extremely energetic solar events, based on solar, stellar, lunar, and terrestrial records
Geoeffectiveness of halo coronal mass ejections
Starspots
The first observed stellar X-ray flare oscillation: Constraints on the flare loop length and the magnetic field
Superflares on the slowly rotating solar-type stars KIC10524994 and KIC07133671?
<i>KEPLER</i>ECLIPSING BINARY STARS. II. 2165 ECLIPSING BINARIES IN THE SECOND DATA RELEASE
The extreme magnetic storm of 1–2 September 1859
The Total Irradiance Monitor (TIM): Science Results
<i>KEPLER MISSION</i> DESIGN, REALIZED PHOTOMETRIC PERFORMANCE, AND EARLY SCIENCE
REVISED STELLAR PROPERTIES OF <i>KEPLER</i> TARGETS FOR THE QUARTER 1-16 TRANSIT DETECTION RUN
Coronal Loop Oscillations Observed with the<i>Transition Region and Coronal Explorer</i>
GLOBAL ENERGETICS OF THIRTY-EIGHT LARGE SOLAR ERUPTIVE EVENTS
<i>Kepler</i>Presearch Data Conditioning II - A Bayesian Approach to Systematic Error Correction
Lectures on Solar Physics
The Relationship Between X‐Ray Radiance and Magnetic Flux
Starspots: A Key to the Stellar Dynamo
Evolution of the solar ionizing flux
1SXPS: A DEEP <i>SWIFT X-RAY TELESCOPE</i> POINT SOURCE CATALOG WITH LIGHT CURVES AND SPECTRA
Kepler Presearch Data Conditioning I—Architecture and Algorithms for Error Correction in Kepler Light Curves
Description of a Singular Appearance seen in the Sun on September 1, 1859
Effects of the March 1989 solar activity
<i>KEPLER</i>ECLIPSING BINARY STARS. I. CATALOG AND PRINCIPAL CHARACTERIZATION OF 1879 ECLIPSING BINARIES IN THE FIRST DATA RELEASE
GLOBAL ENERGETICS OF SOLAR FLARES. I. MAGNETIC ENERGIES
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Original Data Provider (Database)
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Bibliographic ID (NDL)
9483544
NAID
120005756325