Fig. 7.
![Flux appearance and disappearance rates in the solar inter-network at the disk center as a function of time, as observed by Hinode/SOT-NFI (upper and middle panels, respectively). The bottom panel shows the total flux appearance and disappearance rates. [Reproduced from Gošić et al. (2016) by permission of the AAS.] (Color online)](https://oup.silverchair-cdn.com/oup/backfile/Content_public/Journal/pasj/71/5/10.1093_pasj_psz084/2/pasj_71_5_r1_f52.jpeg?Expires=1749936259&Signature=0DHpg0gFiOtAngPPrvPgjcoaFnB0XVfODNbIIlTOHK4IN2YjBFqLnkf4z2n1rHoGqvHHl8BlSFWISod39VzsyDtEbvT~NwvUF5e7HOMW4tqSi8~Vsl8svGtS8PCi8mDueDumeOfF0qgL1eNyQYJvnmPV~7uhjAGE1LVS3FohmAEWHHrr091T5Ycv7p7moC-iDj3LsnZ47Fc-SXB7QxaIev7lCCTJ5DsvxgkUMPjMO1C8Sl8UWZWPTuuN5B1Xqx2rW7rB5roD-JJRbSNJ5pGcpn7OiktiRZ7WRIaYU7E5EVXwAvS9P5OBGh2xtc~0Gp4BkNOAolcP7bMzvxS1~1BlWQ__&Key-Pair-Id=APKAIE5G5CRDK6RD3PGA)
Flux appearance and disappearance rates in the solar inter-network at the disk center as a function of time, as observed by Hinode/SOT-NFI (upper and middle panels, respectively). The bottom panel shows the total flux appearance and disappearance rates. [Reproduced from Gošić et al. (2016) by permission of the AAS.] (Color online)
