Solar Geophysical Activity Report and Forecast march 2015

Solar Activity

.24 hr Summary...
Solar activity remained at low levels. There were several C-class/Sf
flares observed, many of which originated from an unnumbered region on
the southeast limb and most from Region 2305. Region 2305 (S08E19,
Ekc/beta-gamma-delta) continued to grow in area, maintained an increased
magnetic complexity, and produced the largest flare of the period, a
C8/1n flare at 25/0446 UTC. No Earth directed CMEs were observed with
available imagery and observation data.

.Forecast...
Solar activity is likely to be at low levels with a chance for an
M-class (R1-Minor) flare for the forecast period (26-28 Mar).

Energetic Particle

.24 hr Summary...
The greater than 2 MeV electron flux at geosynchronous orbit was once
again at high levels. The greater than 10 MeV proton flux at
geosynchronous orbit returned to near background values.

.Forecast...
The greater than 2 MeV electron flux at geosynchronous orbit is forecast
to remain at high levels through day three (26-28 Mar). The greater than
10 MeV proton flux at geosynchronous orbit is expected to be at or near
background conditions for days one through three (26-28 Mar).

Solar Wind

.24 hr Summary...
The solar wind environment at the ACE spacecraft reflected the continued
influence of a positive polarity high speed solar wind stream.  Wind
speed hovered between 580 and 500 km/s. Bt was at or below 7 nT while
Bz remained at or above -5 nT.  Phi was mostly positive.

.Forecast...
The high speed wind stream is expected to gradually decrease through
days one and two (26-27 Mar). A solar sector boundary crossing (SSBC) to
a negative Phi orientation is forecast late on day two. A recurrent
negative polarity solar wind structure is expected to become
geoeffective, with velocities near 700 km/s expected for day three (28
Mar).

Geospace

.24 hr Summary...
The geomagnetic field ranged from quiet to active levels in response to
the continued influence of the positive polarity high speed solar wind
stream.

.Forecast...
The geomagnetic field is expected to range from quiet to unsettled
levels through day one (26 Mar).  Unsettled to active conditions are
expected on day two (27 Mar) with the SSBC. Day three (28 Mar) is
forecast to see activity as high as a minor storm due to the onset of
the recurrent negative polarity high speed stream.

Solar Geophysical Activity Report and Forecast Oct 23 2014

Solar Geophysical Activity Report and Forecast
SDF Number 296 Issued at 2200Z on 23 Oct 2014


IA.  Analysis of Solar Active Regions and Activity from 22/2100Z to
23/2100Z: Solar activity has been at moderate levels for the past 24
hours. The largest solar event of the period was a M1 event observed at
23/0950Z from Region 2192 (S14W06). There are currently 5 numbered
sunspot regions on the disk.
IB.  Solar Activity Forecast: Solar activity is expected to be moderate
with a chance for X-class flares on days one, two, and three (24 Oct, 25
Oct, 26 Oct).

IIA.  Geophysical Activity Summary 22/2100Z to 23/2100Z: The geomagnetic
field has been at quiet to active levels for the past 24 hours. Solar
wind speed, as measured by the ACE spacecraft, reached a peak speed of
503 km/s at 22/2349Z. Total IMF reached 6 nT at 23/2100Z. The maximum
southward component of Bz reached -5 nT at 23/1717Z. Electrons greater
than 2 MeV at geosynchronous orbit reached a peak level of 6898 pfu.
IIB.  Geophysical Activity Forecast: The geomagnetic field is expected
to be at unsettled to active levels on day one (24 Oct) and quiet to
unsettled levels on days two and three (25 Oct, 26 Oct). Protons have a
chance of crossing threshold on days one through three (24-26 Oct).

III.  Event probabilities 24 Oct-26 Oct
Class M    85/85/85
Class X    45/45/45
Proton     35/40/45
PCAF       green

IV.  Penticton 10.7 cm Flux
Observed           23 Oct 227
Predicted   24 Oct-26 Oct 230/230/230
90 Day Mean        23 Oct 138

V.  Geomagnetic A Indices
Observed Afr/Ap 22 Oct  010/011
Estimated Afr/Ap 23 Oct  008/010
Predicted Afr/Ap 24 Oct-26 Oct  012/015-009/010-007/010

VI.  Geomagnetic Activity Probabilities 24 Oct-26 Oct
A.  Middle Latitudes
Active                30/25/20
Minor Storm           15/05/05
Major-severe storm    01/01/01
B.  High Latitudes
Active                15/15/15
Minor Storm           30/30/25
Major-severe storm    45/30/25

Oct 23 2014, Current Solar Flare Activity, current solar flares, solar wind activity, Latest Solar Flare Activity, solar flare activity, solar activity 2014, 2014, oct 2014

Good morning. Here is an updated look at the visible solar disk, along with active region (AR) 2192 on Thursday. Solar activity during the past 24 hours was high. AR 2192 was responsible for a strong X1.6 solar flare on Wednesday peaking at 14:28 UTC. Unfortunately for sky watchers, the latest event again failed to produce a coronal mass ejection (CME). The active region also produced a few M-Flares, including an M1.1 at 09:50 UTC Thursday morning. AR 2192 expanded to a size of 2700 millionths which puts it on par, at least in terms of total area coverage with legendary Cycle 23 sunspot 486 from October 2003. AR 2192 is now in a near perfect geoeffective position for Earth directed eruptions. The cluster still maintains a complex Beta-Gamma-Delta magnetic configuration and could produce additional moderate to strong solar flares. Elsewhere, a region located near the southeast limb produced an M1.4 flare at 15:57 UTC Wednesday, along with a handful of C-Flares. All other visible regions are currently stable.

Current Solar Flare Activity oct 15 2013

Updated 10/16/2013 @ 00:05 UTC
Impulsive M-Flare
Sunspot 1865 produced an impulsive M1.3 solar flare at 23:36 UTC Tuesday evening. Impulsive flares are not generally known to produce large coronal mass ejections, however I will provide further updates if necessary. Continue to monitor this region for further flare activity. Image below by SDO using the 094 angstroms channel.

Solar Activity

.24 hr Summary...
Solar activity was at moderate levels. Region 1865
(S21W21,Dao/beta-gamma-delta) produced M1 flares at 15/0838 UTC and
15/2336 UTC. An associated coronal mass ejection (CME) subsequently
occurred from the 15/0838 UTC flare. The event appeared narrow and off
plane from an earthward trajectory. The filament related CME from around
15/00 UTC was also determined unlikely to be a geoeffective transient.
Region 1865 maintained an east/west inversion line running through the
adjoined leader spots as well as a beta-gamma-delta configuration.
Region 1861 (S10W45, Dho/beta) showed slight growth in its intermediate
spots and was responsible for multiple C-class flares. A new region
(1872) was numbered near S15E67, and appeared to be  magnetically simple
and inactive.

.Forecast...
Solar activity is expected to be low with a chance for an M-class (R1-R2
Minor to Moderate) flare for the forecast period.  The most likely
regions for M-class flare activity continue to be Regions 1861 and 1865.

Energetic Particle

.24 hr Summary...
The greater than 2 MeV electron flux at geosynchronous orbit was at
normal to moderate levels.  The greater than 10 MeV proton flux at
geosynchronous orbit was at background levels.

.Forecast...
The greater than 2 MeV electron flux at geosynchronous orbit is expected
to be at normal to moderate levels for the forecast period (16-18 Oct). 
The greater than 10 MeV proton flux at geosynchronous orbit is expected
to remain at background levels.

Solar Wind

.24 hr Summary...
Solar wind parameters continued to indicate the influence of a coronal
hole high-speed stream (CH HSS). Speed ranged from 460 to 575 km/s
during the period. IMF total field decreased from a high around 12 nT
early in the period to lows of around 2 nT during the latter half of the
period. Intermittent incidences of negative Bz occurred throughout the
period.

.Forecast...
Enhanced solar wind speed and IMF variability are expected to persist
for the next three days (16-18 Oct) from combined effects of residual CH
HSS and the anticipated arrival of the CME from 13 Oct late on day one
(16 Oct).

Geospace

.24 hr Summary...
The geomagnetic field was at quiet to active levels due to CH HSS and
possible weak CME effects.

.Forecast...
The geomagnetic field is expected to be at quiet to active levels for
day one (16 Oct) due to residual CH HSS conditions early before the
anticipated arrival of the weak CME from 13 October late on day one.
Quiet to active conditions are expected to persist on day 2 (17
Oct).  By day three (18 Oct), conditions are expected to decrease to
mostly quiet levels with unsettled periods as CH HSS and CME effects
wane.

latest solar flare activity august 23 2013

Analysis of Solar Active Regions and latest solar flare activity august 23 2013from 22/2100Z to
23/2100Z: Solar activity has been at low levels for the past 24 hours.
The largest solar event of the period was a C1 event observed at
22/2207Z from Region 1828 (N14E26). There are currently 9 numbered
sunspot regions on the disk.

 IB.  Solar Activity Forecast: Solar activity is expected to be low with
a slight chance for an M-class flare on day one (24 Aug) and expected to
be low on days two and three (25 Aug, 26 Aug).


IIA.  Geophysical Activity Summary 22/2100Z to 23/2100Z: The geomagnetic
field has been at quiet to active levels for the past 24 hours. Solar
wind speed, as measured by the ACE spacecraft, reached a peak speed of
593 km/s at 22/2215Z. Total IMF reached 7 nT at 22/2100Z. The maximum
southward component of Bz reached -5 nT at 22/2205Z. Electrons greater
than 2 MeV at geosynchronous orbit reached a peak level of 1857 pfu.

IIB.  Geophysical Activity Forecast: The geomagnetic field is expected
to be at unsettled to minor storm levels on day one (24 Aug), quiet to
minor storm levels on day two (25 Aug) and quiet to unsettled levels on
day three (26 Aug). 

Solar activity was low.  Region 1820 (S12W73, Cao/beta) produced a C1 at
23/1557 UTC, which was the largest event of the period.  Region 1830
(S05W64, Dao/beta) showed minor growth while the other regions on the
disk were either stable or decaying.  A narrow coronal mass ejection
(CME) from Region 1820 was observed on LASCO C2 coronagraph imagery at
23/0048 UTC, but was not Earth-directed.

.Forecast...
Solar activity is expected to be low with a slight chance for M-class
flares on day one (24 Aug).  Solar activity is expected to be low for
days two and three (25 - 26 Aug).

Energetic Particle

.24 hr Summary...
The greater than 2 MeV electron flux at geosynchronous orbit was at
normal to high levels, reaching a maximum value of 1,860 pfu at 23/1710
UTC.  The greater than 10 MeV proton flux at geosynchronous orbit was at
background levels.

.Forecast...
The greater than 2 MeV electron flux at geosynchronous orbit is expected
to be at normal to high levels for the next three days (24 - 26 Aug). 
The greater than 10 MeV proton flux at geosynchronous orbit is expected
to remain at background levels for the next three days (24 - 26 Aug).

Solar Wind

.24 hr Summary...
Solar wind parameters, measured at ACE, were indicative of waning
coronal hole high speed stream (CH HSS) influence.  Solar wind speed
steadily decreased from initial values near 560 km/s to end-of-period
values near 475 km/s.  The total field strength ranged from 6 nT to 2 nT
while the Bz component ranged from +4 nT to -5 nT.  The phi angle
remained in a predominately positive (away) sector throughout the
period.

.Forecast...
Solar wind speed is expected to increase on day one (24 Aug) and remain
enhanced for days two and three (25 - 26 Aug) with arrival of the 21 Aug
CME and onset of a CH HSS late on day three.

Geospace

.24 hr Summary...
The geomagnetic field was at quiet to active levels.

.Forecast...
With arrival of the 21 Aug CME, the geomagnetic field is expected to be
at unsettled to G1 (Minor) geomagnetic storm levels on day one (24 Aug),
decreasing to quiet to G1 (Minor) geomagnetic storm levels on day two
(25 Aug).  Predominately quiet to unsettled conditions are expected on
day three (26 Aug) with waning CME effects and the onset of a CH HSS.

Solar Active Regions and Activity 17 May 2013

Joint USAF/NOAA Solar Geophysical Activity Report and Forecast
SDF Number 137 Issued at 2200Z on 17 May 2013


IA.  Analysis of Solar Active Regions and Activity from 16/2100Z to
17/2100Z: Solar activity has been at moderate levels for the past 24
hours. The largest solar event of the period was a M3 event observed at
17/0857Z from Region 1748 (N12E23). There are currently 10 numbered
sunspot regions on the disk.

IB.  Solar Activity Forecast: Solar activity is expected to be at
moderate to high levels with a chance for X-class flares on days one,
two, and three (18 May, 19 May, 20 May).



IIA.  Geophysical Activity Summary 16/2100Z to 17/2100Z: The geomagnetic
field has been at quiet to unsettled levels for the past 24 hours. Solar
wind speed, as measured by the ACE spacecraft, reached a peak speed of
431 km/s at 17/0120Z. Total IMF reached 7 nT at 17/1927Z. The maximum
southward component of Bz reached -5 nT at 16/2126Z. Protons greater
than 10 MeV at geosynchronous orbit reached a peak level of 41 pfu at
17/1720Z. Electrons greater than 2 MeV at geosynchronous orbit reached a
peak level of 203 pfu.

IIB.  Geophysical Activity Forecast: The geomagnetic field is expected
to be at quiet to unsettled levels on day one (18 May), quiet to major
storm levels on day two (19 May) and quiet to active levels on day three
(20 May). Protons are expected to continue above threshold levels on
days 1-3 (18-20 May).


III.  Event probabilities 18 May-20 May
Class M    75/75/75
Class X    50/50/50
Proton     99/95/90
PCAF       red

Solar flare Activity Solar Update CME Update 12 May 2013

Joint USAF/NOAA Solar Geophysical Activity Report and Forecast
SDF Number 132 Issued at 2200Z on 12 May 2013


IA.  Analysis of Solar Active Regions and Activity from 11/2100Z to
12/2100Z: Solar activity has been at moderate levels for the past 24
hours. The largest solar event of the period was a M1 event observed at
12/2032Z from a region around the east limb. There are currently 10
numbered sunspot regions on the disk.

IB.  Solar Activity Forecast: Solar activity is expected to be low with
a chance for M-class flares on days one, two, and three (13 May, 14 May,
15 May).


IIA.  Geophysical Activity Summary 11/2100Z to 12/2100Z: The geomagnetic
field has been at quiet levels for the past 24 hours. Solar wind speed,
as measured by the ACE spacecraft, reached a peak speed of 435 km/s at
11/2151Z. Electrons greater than 2 MeV at geosynchronous orbit reached a
peak level of 456 pfu.

IIB.  Geophysical Activity Forecast: The geomagnetic field is expected
to be at quiet to unsettled levels on day one (13 May), quiet levels on
day two (14 May) and quiet to active levels on day three (15 May).


III.  Event probabilities 13 May-15 May
Class M    50/50/50
Class X    05/05/05
Proton     01/01/01
PCAF       green

Updated 05/13/2013 @ 02:10 UTC
X-Class Solar Flare
A major X-Class Solar Flare peaking at X1.7 was observed around an active region hiding off the east limb at 02:15 UTC. This event was also responsible for a strong R3 Level Radio Blackout on the sunlit side of Earth. This region is currently seething with activity and should begin to rotate into view within the next 24 hours. Because of the sunspot location, any associated Coronal Mass Ejection (CME) should be directed away from Earth. Stay Tuned to SolarHam.com for the latest and most up to date Space Weather information.
  M1.9 Flare
A moderate solar flare measuring M1.9 was detected around a new active region off the east limb at 20:32 UTC Sunday evening. This probable sunspot will rotate into view over the next few days. Image by SDO.
SUMMARY: 10cm Radio Burst
Begin Time: 2013 May 13 0208 UTC
Maximum Time: 2013 May 13 0219 UTC
End Time: 2013 May 13 0222 UTC
Duration: 14 minutes
Peak Flux: 320 sfu
Description: A 10cm radio burst indicates that the electromagnetic burst associated with a solar flare at the 10cm wavelength was double or greater than the initial 10cm radio background. This can be indicative of significant radio noise in association with a solar flare. This noise is generally short-lived but can cause interference for sensitive receivers including radar, GPS, and satellite communications.

Solar flare Activity Solar Update CME Update Apr 13 2013

j

Prepared jointly by the U.S. Dept. of Commerce, NOAA,
Space Weather Prediction Center and the U.S. Air Force.
UPDATED 2013 Apr 13 2200 UTC


Joint USAF/NOAA Solar Geophysical Activity Report and Forecast
SDF Number 103 Issued at 2200Z on 13 Apr 2013


IA.  Analysis of Solar Active Regions and Activity from 12/2100Z to
13/2100Z: Solar activity has been at low levels for the past 24 hours.
The largest solar event of the period was a C1 event observed at
13/0334Z from Region 1718 (N21W58). There are currently 7 numbered
sunspot regions on the disk.

IB.  Solar Activity Forecast: Solar activity is expected to be low with
a chance for M-class flares and a slight chance for an X-class flare on
days one and two (14 Apr, 15 Apr) and expected to be low with a chance
for M-class flares on day three (16 Apr).


IIA.  Geophysical Activity Summary 12/2100Z to 13/2100Z: The geomagnetic
field has been at quiet levels for the past 24 hours. Solar wind speed,
as measured by the ACE spacecraft, reached a peak speed of 501 km/s at
12/2336Z. Total IMF reached 5 nT at 12/2240Z. The maximum southward
component of Bz reached -3 nT at 13/0036Z. Protons greater than 10 MeV
at geosynchronous orbit reached a peak level of 10 pfu at 12/2205Z.
Electrons greater than 2 MeV at geosynchronous orbit reached a peak
level of 268 pfu.

IIB.  Geophysical Activity Forecast: The geomagnetic field is expected
to be at unsettled to major storm levels on day one (14 Apr) and quiet
levels on days two and three (15 Apr, 16 Apr). Protons greater than 10
Mev have a chance of crossing threshold on day one (14 Apr) and have a
slight chance of crossing threshold on day two (15 Apr).

Solar flare Activity Solar Update CME Update Apr 11 2013

Joint USAF/NOAA Solar Geophysical Activity Report and Forecast
SDF Number 101 Issued at 2200Z on 11 Apr 2013


IA.  Analysis of Solar Active Regions and Activity from 10/2100Z to
11/2100Z: Solar activity has been at high levels for the past 24 hours.
The largest solar event of the period was a M6 event observed at
11/0716Z from Region 1719 (N10W00). There are currently 6 numbered
sunspot regions on the disk.

IB.  Solar Activity Forecast: Solar activity is expected to be low with
a chance for M-class flares and a slight chance for an X-class flare on
days one, two, and three (12 Apr, 13 Apr, 14 Apr).


IIA.  Geophysical Activity Summary 10/2100Z to 11/2100Z: The geomagnetic
field has been at quiet levels for the past 24 hours. Solar wind speed,
as measured by the ACE spacecraft, reached a peak speed of 507 km/s at
11/1243Z. Total IMF reached 7 nT at 11/0712Z. The maximum southward
component of Bz reached -4 nT at 11/0916Z. Protons greater than 10 MeV
at geosynchronous orbit reached a peak level of 114 pfu at 11/1645Z.
Protons greater than 100 MeV at geosynchronous orbit reached a peak
level of 2 pfu at 11/1400Z. Electrons greater than 2 MeV at
geosynchronous orbit reached a peak level of 385 pfu.

IIB.  Geophysical Activity Forecast: The geomagnetic field is expected
to be at quiet levels on day one (12 Apr), quiet to major storm levels
on day two (13 Apr) and unsettled to major storm levels on day three (14
Apr). Protons are expected to cross threshold on day one (12 Apr), have
a chance of crossing threshold on day two (13 Apr) and have a slight
chance of crossing threshold on day three (14 Apr).


III.  Event probabilities 12 Apr-14 Apr
Class M    50/50/50
Class X    15/15/15
Proton     99/30/10
PCAF       red

CME Update: A bright full-halo Coronal Mass Ejection (CME) is visible within the new Lasco imagery. It appears that a bulk of the plasma is directed towards the east, however there also appears to be a fair sized Earth directed

A moderately strong solar flare was observed around Sunspot 1719 at 07:16 UTC. A Coronal Mass Ejection (CME) was generated and looks to be directed mostly to the east. There is however an Earth directed component that could deliver at least a glancing blow or more to our geomagnetic field within 48 hours. Energetic Proton Levels streaming past Earth are on the rise following the flare event. A minor to moderate S2 Level Radiation Storm is currently in progress.

A couple more solar flares of the smaller variety were observed following the initial M6.5 event. A minor flare measuring C4.2 was detected around 1721 in the southeast quadrant at 10:13 UTC. Departed Sunspot 1713 off the west limb produced a flare measuring C6.2 at 10:46 UTC. SolarSoft has the flare at C6.3.

Solar Activity Forecast: Solar activity

Joint USAF/NOAA Solar Geophysical Activity Report and Forecast
SDF Number 28 Issued at 2200Z on 28 Jan 2013


IA.  Analysis of Solar Active Regions and Activity from 27/2100Z to
28/2100Z: Solar activity has been at low levels for the past 24 hours.
The largest solar event of the period was a C1 event observed at
28/1834Z from Region 1660 (N13, L=065) which is about a day beyond West
limb. There are currently 4 numbered sunspot regions on the disk.

IB.  Solar Activity Forecast: Solar activity is expected to be at very
low with a chance for C-class flares on days one, two, and three (29
Jan, 30 Jan, 31 Jan).


IIA.  Geophysical Activity Summary 27/2100Z to 28/2100Z: The geomagnetic
field has been at quiet levels for the past 24 hours. Solar wind speed,
as measured by the ACE spacecraft, reached a peak speed of 445 km/s at
28/0310Z and was slowly decreasing throughout the period.

IIB.  Geophysical Activity Forecast: The geomagnetic field is expected
to be at quiet levels for the next three days (29 Jan, 30 Jan, 31 Jan).


III.  Event probabilities 29 Jan-31 Jan
Class M    05/05/05
Class X    01/01/01
Proton     01/01/01
PCAF       green

Current Solar Flare Activity on 12/21/2012

12 21 2012, or December 21 2012 is often a date associated with the finish with the world. This date, 12 21 2012, arrives mostly from the extended count in the Mayan calendar. The Mayans for reasons unidentified were quite innovative within the study of astronomy. Their calendar is really many calendars in one. The calendar referred to as the extended count is the one which notes 12 21 2012 since the conclude in the earth as we realize it.The reason for this day is quite problematic. On December 21, 2012 or 12 21 2012, for the 1st time in 26000 a long time, the sun will conjunct the milky way, along with the elliptical plane

The Mayan Calendar has left us with a profound mystery. Academia, science and the clergy have labored long over the question as to why the calendar was extrapolated into the 21st century and why, on December 21st, 2012, it abruptly ends?

Eschatology could be the research in the stop of life on earth. There are several speculations just before 12 21 2012. One of many most recent instances for such speculation was referred to as Y2K. Though Y2K primarily was regarding computer systems, some noticed it like an indication from the end occasions. I think that a lot of folks experience that 2012 could be the conclude for any range of good reasons. Very first of all, guilt could play a part within this. Surely the human race has considerably to be ashamed of. Furthermore, many weather conditions changes and adjustments to our environment have taken spot. We've got noticed what alterations in local weather can do to our civilization in storms such as Katrina. Moreover to all of this, considerably of the world is facing horrible financial conditions

As the predicted date of the end of the world, that is the 12 21 2012 Polar Shift, draws nearer, the more we need to focus our attention on the innumerable things that could possibly happen on planet Earth. Theorists and experts alike have in fact, enumerated a number of possibilities that can take place come year 2012. Although there is no scientific proof to confirm that all such predictions will surely come true, there are countless of predictions about the possibilities that can happen in the envisaged Doomsday of 2012. Here are just a few of these possibilities that you should know regarding the December 12, 2012 Polar Shift so that you can be prepared as to what can possibly occur during such time:
1. Asteroid, Meteor And Comet
First and foremost, experts and theorists predict the possibility of experiencing an orbit which may culminate by colliding with our planet earth in the year 2012. While this may be the most predictable catastrophe come 2012, it will still be good to not doubt it and instead, equip ourselves with the appropriate survival kit to make sure that we stay alive even if the predicted phenomenon finally takes place.
2. Coronal Mass Ejection From The Sun
For those who may not know it, the CME or Coronal Mass Ejection which came from the sun and caused the year 1859's solar storm, is actually true. Such event took place during the month of September of 1859 bringing about a failure in the telegraph systems from corner to corner of North America as well as Europe. The same event is in fact, predicted to occur in the year 2012 when the end of the world is envisaged to take place. What is more, it is also forecast that there are going to be huge storms bringing such massive power blackouts at the same time, the wreckage of satellites.
3. Magnetic Pole Shift
Polar reversals such as the 12 21 2012 Polar Shift are predicted to be occurring at a time gap of 400,000 years. In fact, the most current polar shift that occurred happened about 730,000 years ago and not too many people even know about it. You see, even our scientists still lack the knowledge about polar reversals, in the same manner that they are not so sure until now, about how such magnetic fields are generated. Although they are able to predict that geomagnetic reversals such as the 12 21 2012 Polar Shift, would take about hundreds and hundreds of years to take place and that they actually cause no harm at all. But then this has been disputed as it was found out that polar shifts can actually take place in just a snap of the fingers, yes, as in anytime.
4. Explosion From The Black Hole
Another possibility that is expected to take place after a polar shift in planet Earth is the possible danger of a Galactic core explosion, or what is simply an explosion from the Black Hole at the center or middle of our galaxy. It is expected that such incident will bring about some cosmic ray super waves that would be gestured by a burst of gamma rays. These bursts are actually believed to cause the massively destructive tsunamis in our planet.

 There are many theories regarding just what will transpire on 12 21 2012. Several feel that solar flare activity will improve significantly and that a huge solar flare will strike the earth causing destruction. Other theories incorporate the earth being struck by a mystery planet or asteroid known as planet x. Nonetheless other speculations say that the earths wobble on its axis, will trigger drastic modifications while in the earths weather and environment creating mass destruction by components this kind of as tidal waves. Even though there are many diverse theories,several authorities agree that "something" will occur in 2012.Some people imagine that 2012 will mark the finish of everyday living on our planet, even though other people do not. Some see it as being a time of drastic change and survival for those that transform spiritually. So called specialists link the Mayan calendar with other prophesies these as Nostradamus, as well as the end occasions explained while in the Bible inside the guide of Revelations. Nevertheless there is certainly little or no if any connection to that actual day in both of these resources.
.
All of this could look just like the occasions preceding the end times.Considering that considerably with the info on 12 21 2012 is speculation, it is critical to have your data from a trustworthy resource. With this way you may make intelligent and educated decisions on what you feel. There are numerous authorities that sense 12 21 2012 is often a time for survival and good change. Let us hope that's true. 2012 Specifics