Loading ...
Sorry, an error occurred while loading the content.

Re: Roman fall not the sun

Expand Messages
  • Pawnfart
    What I mean by properly observed actually takes what you are saying into account. The Gaia issue is thus--when cirrus conditions improve, SSTs warm. SSTs
    Message 1 of 702 , Jan 5, 2002
    • 0 Attachment
      What I mean by "properly observed" actually takes
      what you are saying into account. The Gaia issue is
      thus--when cirrus conditions improve, SSTs warm. SSTs hence
      denote electrical conditions where the specific
      conductivity of the oceans increases, at least in terms of
      extremes. What that means is that oceans begin to become
      more electrically significant as far as the cirrus
      enhancement. The best example is ENSO, which happens to
      decrease in frequency during the cold periods of the LIA.
      OTOH, when ocean SSTs drop, flaring from the top of the
      atmosphere becomes more significant. Hence, flaring should
      be correlated MORE with clouds, and clouds more
      correlated with hiding the flaring activity for those with
      poor instrumentation. Get it?<br><br>But the final
      kicker is that you can't find mechanism going the other
      way with respect to Keeling Whorf and moon earth
      depressurization values on methane hydrate fields, and drops in
      insulation or specific conducitivty that this would cause,
      decreasing cirrus enhancement. Keeling Whorf is much more
      reliable because the orbital physics of the moon and earth
      is classical and observable on all timescales. The
      measures of flaring are only recently reliable.
    • b1blancer_29501
      On Feb 28th, the Interplanetary Magnetic Field swung to a strong south-pointing orientation. That, coupled with an elevated solar wind speed and density,
      Message 702 of 702 , Mar 1 9:47 PM
      • 0 Attachment
        On Feb 28th, the Interplanetary Magnetic Field
        swung to a strong south-pointing orientation. That,
        coupled with an elevated solar wind speed and density,
        triggered a G-1 class geomagnetic storm. The result was
        some high latitude aurora. See this link for a
        photgraph of aurora observed over Quebec :
        <a href=http://www.spaceweather.com/aurora/images/01mar02/Moussette2.jpg target=new>http://www.spaceweather.com/aurora/images/01mar02/Moussette2.jpg</a> . As of right now, there are 3 sunspot regions,
        namely 9839, 9842, and 9845, that appear to be capable
        of producing M-class flares. Regions 9839 and 9842
        are close to rotating out of view over the western
        limb of the solar disk. Sunspot region 9845, however,
        is close to the sun's central meridian. A rather
        large coronal hole is also approaching the sun's
        central meridian, and coming into an Earth-pointing
        position. High speed colar wind gusts are likely around the
        first of next week.<br><br>The current solar and
        geomagnetic conditions are :<br><br>NOAA sunspot number :
        153<br>SFI : 188<br>A index : 10<br>K index : 1<br><br>Solar
        wind speed : 372.3 km/sec<br>Solar wind density : 4.4
        protons/cc<br>Solar wind pressure : 1.1 nPa<br><br>IMF : 8.4
        nT<br>IMF Orientation : 0.7 nT North<br><br>Conditions for
        the last 24 hours : <br>Solar activity was low. The
        geomagnetic field was quiet to unsettled. Stratwarm Alert
        exists Friday.<br><br>Forecast for the next 24 hours
        :<br>Solar activity will be low to moderate. The geomagnetic
        field will be quiet to unsettled.<br><br>Solar Activity
        Forecast :<br>Solar activity is expected to be low to
        moderate for the next three days. Region 9845 is a
        possible source for isolated M-class
        flares.<br><br>Geomagnetic activity forecast :<br>Geomagnetic field activity
        is expected to be mainly quiet to unsettled, until
        the onset of high speed stream effects from a
        recurrent coronal hole begin to develop by day three of the
        forecast period. Isolated active conditions are
        anticipated thereafter.<br><br>Recent significant solar flare
        activity :<br>None
      Your message has been successfully submitted and would be delivered to recipients shortly.