by neufer » Fri Aug 04, 2017 1:33 pm
http://adsabs.harvard.edu/abs/2011JBAA..121...19R wrote:
<<As well as the Great Red Spot, Jupiter sometimes presents one or more Little Red Spots (LRSs) in various latitudes. An LRS is often seen in the North North Temperate Zone (NNTZ), but the frequency and properties of these ovals have never been studied in detail. Here we review all our records of the red, white, and methane-bright anticyclonic ovals in the NNTZ. There is a simple conclusion: A single LRS, which we name NN-LRS-1, has persisted from 1993 to 2009. It has varied in colour between red and off-white, but has been methane-bright throughout these years. This now ranks among the most long-lived spots ever recorded on the planet. There is always at least one other oval in this latitude. This was a second methane-bright LRS from 1994-1997, and there was also a smaller LRS in 2006. The other ovals are all white; two have lasted for four years or more and were sometimes methane-bright; others have had shorter lives and were not. These results suggest that red colour, and the high-level haze that accompanies it, are correlated with the size and longevity of the oval. All these ovals have variable speeds, alternating irregularly between slow (~ 1°/month in System II longitude) and fast (~ 12°/month). The latitudes of the ovals range from 40 to 41.5°N, and correlate closely with their instantaneous speeds. However the larger, longer-lived ovals (especially the LRS) are centred systematically further south than the smaller white ovals, because they distort the retrograding jetstream more deeply. Similar behaviour in other domains on the planet explains how ovals of different sizes move with a single slow current while also being sensitive to the zonal speed gradient.
An oval at 60°S shows very similar behaviour and has probably existed since 1994 or earlier.>>
[quote="APOD Robot"][url=https://apod.nasa.gov/apod/ap170804.html][img]https://apod.nasa.gov/apod/calendar/S_170804.jpg[/img] [size=150]North North Temperate Zone Little Red Spot[/size][/url]
[b] Explanation: [/b] On July 11, the Juno spacecraft once again swung near the turbulent Jovian cloud tops. On its seventh orbital closest approach this [url=https://apod.nasa.gov/apod/ap170603.html]perijove passage[/url] brought Juno within 3,500 kilometers of the Solar System's largest planetary atmosphere. Near perijove the rotating [url=https://www.missionjuno.swri.edu/junocam/processing#AboutJunoCamImages]JunoCam[/url] was able to record [url=https://www.facebook.com/thenightskyguy/posts/10154892042387775]this stunning, clear view[/url] of one of Jupiter's [url=http://www.planetary-astronomy-and-imaging.com/en/new-red-spot-on-jupiter/]signature vortices.[/url] About 8,000 kilometers in diameter, the anticyclonic storm system was spotted in Jupiter's [url=https://en.wikipedia.org/wiki/Atmosphere_of_Jupiter#Specific_bands]North North Temperate Zone[/url] in the 1990s. That makes it about half the size of an older and better known Jovian anticyclone, the [url=https://apod.nasa.gov/apod/ap170715.html]Great Red Spot[/url], but only a little smaller than planet Earth. At times taking on reddish hues, the enormous storm system is fondly known as a [url=http://adsabs.harvard.edu/abs/2011JBAA..121...19R]North North Temperate Zone Little Red Spot[/url].[/quote]
[c]An anticyclonic storm system [b][u][color=#0000FF]was[/color][/u][/b] indeed spotted in Jupiter's [url=https://en.wikipedia.org/wiki/Atmosphere_of_Jupiter#Specific_bands]North North Temperate Zone[/url] [b][u][color=#0000FF]in the 1990s[/color][/u][/b] [b][u]
[color=#FF0000]AND THIS APOD IS'NT IT[/color][/u][/b] :!:[/c]
[quote=" http://adsabs.harvard.edu/abs/2011JBAA..121...19R"]
[float=left][img3="[color=#0000FF][b][size=150]Today's APOD is of the 23+ year old South TZ LRS[/size][/b][/color]"]https://upload.wikimedia.org/wikipedia/commons/2/23/Jupiter_cloud_bands.svg[/img3][/float]<<As well as the Great Red Spot, Jupiter sometimes presents one or more Little Red Spots (LRSs) in various latitudes. An LRS is often seen in the North North Temperate Zone (NNTZ), but the frequency and properties of these ovals have never been studied in detail. Here we review all our records of the red, white, and methane-bright anticyclonic ovals in the NNTZ. There is a simple conclusion: A single LRS, which we name NN-LRS-1, has persisted from 1993 to 2009. It has varied in colour between red and off-white, but has been methane-bright throughout these years. This now ranks among the most long-lived spots ever recorded on the planet. There is always at least one other oval in this latitude. This was a second methane-bright LRS from 1994-1997, and there was also a smaller LRS in 2006. The other ovals are all white; two have lasted for four years or more and were sometimes methane-bright; others have had shorter lives and were not. These results suggest that red colour, and the high-level haze that accompanies it, are correlated with the size and longevity of the oval. All these ovals have variable speeds, alternating irregularly between slow (~ 1°/month in System II longitude) and fast (~ 12°/month). The latitudes of the ovals range from 40 to 41.5°N, and correlate closely with their instantaneous speeds. However the larger, longer-lived ovals (especially the LRS) are centred systematically further south than the smaller white ovals, because they distort the retrograding jetstream more deeply. Similar behaviour in other domains on the planet explains how ovals of different sizes move with a single slow current while also being sensitive to the zonal speed gradient.[size=150] [b][u][color=#0000FF]An oval at 60°S shows very similar behaviour and has probably existed since 1994 or earlier.[/color][/u][/b][/size]>>[/quote]