Fig. 9.
![Synoptic diagrams of the unsigned longitudinal apparent flux density ($|B^{\rm L}_{\rm app}|$) as a function of time and latitude: (a) all longitudinal flux; (b) inter-network longitudinal flux; (c) same as panel (b) but displayed against disk angle rather than solar latitude; (d) same as panel (c) but limited to the very weak inter-network with $|B^{\rm L}_{\rm app}| \lt $ 20 Mx cm−2. [Figure 4 from Lites, Centeno, and McIntosh (2014).] (Color online)](https://oup.silverchair-cdn.com/oup/backfile/Content_public/Journal/pasj/71/5/10.1093_pasj_psz084/2/pasj_71_5_r1_f54.jpeg?Expires=1750035708&Signature=cL1cGxlVHkrd5UCMmvUwlXwGjwW6pTzpeF-LQWVYJPW8PqPxurBsgnVIS1heeJnvmEjOzwHXysmF0WmzGSVvs4BJPlDStagL8IxRl~Tx8pUT2norpCWlyxCw62AMMNjiRE9us5dsP5dgRoBGS1ABs6N~pCQeziBSO6fz~E3z2wPS3j6LdvHR3qMSt7PE3AScq-AvFs~2STu77SAFD7M2fWJnCb4rEFex6PnvEQti7FWKi3fY-9zvZPnPWf72i~nV409hct2Qu1~NpRBPy5gLMMQZnRraXY2LCXM5lL1UBz2SsYOCRcqbr0Zno0psUnyEFa6cpnk9bT6Iu~VxvOMXbQ__&Key-Pair-Id=APKAIE5G5CRDK6RD3PGA)
Synoptic diagrams of the unsigned longitudinal apparent flux density (|$|B^{\rm L}_{\rm app}|$|) as a function of time and latitude: (a) all longitudinal flux; (b) inter-network longitudinal flux; (c) same as panel (b) but displayed against disk angle rather than solar latitude; (d) same as panel (c) but limited to the very weak inter-network with |$|B^{\rm L}_{\rm app}| \lt $| 20 Mx cm−2. [Figure 4 from Lites, Centeno, and McIntosh (2014).] (Color online)
