000004150 001__ 4150
000004150 005__ 20190211122835.0
000004150 037__ $$aDATASET-2019-0051
000004150 100__ $$aWest, Matthew
000004150 245__ $$aSWAP Carrington Rotation Files
000004150 260__ $$c2018
000004150 520__ $$aA Carrington Rotation is a period of time chosen to represent one rotation of the Sun, allowing the comparison of features such as sunspot groups or active regions. A period of 27.28 days was chosen to represent a single rotation that largely resembles the recurrence time of features near the equator. Each movie has a cadence of roughly 40 minutes, and each image is comprised of a median stacked set of smoothed SWAP images. By managing the images in this we're able to enhance the signal in the solar corona. The solar corona (the outer solar atmosphere) is seen as the ethereal region of the image surrounding the solar disk. During periods of high acitivty this region can be extremely dynamic showing complicated magnetic structures, as can be seen in the image below.
000004150 536__ $$a3ESA_PROBA2SOC/$$c3ESA_PROBA2SOC/$$f3ESA_PROBA2SOC
000004150 594__ $$aNO
000004150 700__ $$aStegen, Koen
000004150 700__ $$aNicula, Bogdan
000004150 700__ $$aD'Huys, Elke
000004150 700__ $$aBerghmans, David
000004150 700__ $$aSeaton, Daniel
000004150 700__ $$aDominique, Marie
000004150 700__ $$aBonte, Katrien
000004150 700__ $$aOhara, Jennifer
000004150 700__ $$aWauters, Laurence
000004150 8560_ $$fmatthew.west@observatoire.be
000004150 85642 $$ahttp://proba2.oma.be/swap/data/carrington_rotations/
000004150 980__ $$aDATASET