Non-homogeneous Behaviour of the Spatial Distribution of Macrospicules

Abstract

In this paper the longitudinal and latitudinal spatial distribution of macrospicules is examined. We found a statistical relationship between the active longitude determined by sunspot groups and the longitudinal distribution of macrospicules. This distribution of macrospicules shows an inhomogeneity and non-axysimmetrical behaviour in the time interval from June $2010$ until December $2012$ covered by observations of the Solar Dynamic Observatory (SDO) satellite. The enhanced positions of the activity and its time variation has been calculated. The migration of the longitudinal distribution of macrospicules shows a similar behaviour as that of the sunspot groups.

References in corpus (4)

• Observational Signatures of Simulated Reconnection Events in the Solar Chromosphere and Transition Region
• Origin of Macrospicule and Jet in Polar Corona by A Small-scale Kinked Flux-Tube
• Migration and Extension of Solar Active Longitudinal Zones
• Blue straggler evolution caught in the act in the Large Magellanic Cloud globular cluster Hodge 11

Cited by in corpus (5)

• Systematic variations of macrospicule properties observed by SDO/AIA over half a decade
• What is a Macrospicule?
• Untwisting Jets Related to Magnetic Flux Cancellation
• On Quasi-biennial oscillations in chromospheric macrospicules and their potential relation to global solar magnetic field
• Quasi-biennial oscillations in the cross-correlation of properties of macrospicules