Probing the Effect of Cadence on the Estimates of Photospheric Energy and Helicity Injections in Eruptive Active Region NOAA AR 11158

Näytä kaikki kuvailutiedot



Pysyväisosoite

http://hdl.handle.net/10138/303869

Lähdeviite

Lumme , E , Kazachenko , M D , Fisher , G H , Welsch , B T , Pomoell , J & Kilpua , E K J 2019 , ' Probing the Effect of Cadence on the Estimates of Photospheric Energy and Helicity Injections in Eruptive Active Region NOAA AR 11158 ' , Solar Physics , vol. 294 , no. 6 , 84 . https://doi.org/10.1007/s11207-019-1475-x

Julkaisun nimi: Probing the Effect of Cadence on the Estimates of Photospheric Energy and Helicity Injections in Eruptive Active Region NOAA AR 11158
Tekijä: Lumme, E.; Kazachenko, M. D.; Fisher, G. H.; Welsch, B. T.; Pomoell, J.; Kilpua, E.K.J.
Tekijän organisaatio: Space Physics Research Group
Particle Physics and Astrophysics
Department of Physics
Päiväys: 2019-06-27
Kieli: eng
Sivumäärä: 40
Kuuluu julkaisusarjaan: Solar Physics
ISSN: 1573-093X
DOI-tunniste: https://doi.org/10.1007/s11207-019-1475-x
URI: http://hdl.handle.net/10138/303869
Tiivistelmä: We study how the input-data cadence affects the photospheric energy and helicity injection estimates in eruptive NOAA Active Region 11158. We sample the novel 2.25-minute vector magnetogram and Dopplergram data from the Helioseismic and Magnetic Imager (HMI) instrument onboard the Solar Dynamics Observatory (SDO) spacecraft to create input datasets of variable cadences ranging from 2.25 minutes to 24 hours. We employ state-of-the-art data processing, velocity, and electric-field inversion methods for deriving estimates of the energy and helicity injections from these datasets. We find that the electric-field inversion methods that reproduce the observed magnetic-field evolution through the use of Faraday's law are more stable against variable cadence: the PDFI (PTD-Doppler-FLCT-Ideal, where PTD refers to Poloidal-Toroidal Decomposition, and FLCT to Fourier Local Correlation Tracking) electric-field inversion method produces consistent injection estimates for cadences from 2.25 minutes up to two hours, implying that the photospheric processes acting on time scales below two hours contribute little to the injections, or that they are below the sensitivity of the input data and the PDFI method. On other hand, the electric-field estimate derived from the output of DAVE4VM (Differential Affine Velocity Estimator for Vector Magnetograms), which does not fulfill Faraday's law exactly, produces significant variations in the energy and helicity injection estimates in the 2.25 minutes - two hours cadence range. We also present a third, novel DAVE4VM-based electric-field estimate, which corrects the poor inductivity of the raw DAVE4VM estimate. This method is less sensitive to the changes of cadence, but it still faces significant issues for the lowest of considered cadences (two hours). We find several potential problems in both PDFI- and DAVE4VM-based injection estimates and conclude that the quality of both should be surveyed further in controlled environments.
Avainsanat: BOUNDARY
Corona
ELECTRIC-FIELDS
FIT
Helicity
LOCAL CORRELATION TRACKING
Magnetic fields
VECTOR MAGNETOGRAMS
VELOCITY
active
corona
magnetic
models
observations
photosphere
115 Astronomy, Space science
Vertaisarvioitu: Kyllä
Tekijänoikeustiedot: cc_by
Pääsyrajoitteet: openAccess
Rinnakkaistallennettu versio: publishedVersion


Tiedostot

Latausmäärä yhteensä: Ladataan...

Tiedosto(t) Koko Formaatti Näytä
Lumme2019_Artic ... heEffectOfCadenceOnThe.pdf 4.410MB PDF Avaa tiedosto

Viite kuuluu kokoelmiin:

Näytä kaikki kuvailutiedot