Related Links Recommended Reading - An Interpretation of the Fields of Force and How they are Utilized in Culture and for ARV accuracy Tachyonic Time Camera? - Possible detection of tachyon monopoles in photographic emulsions
Recommended Reading - Synchronization of Human Autonomic Nervous System Rhythms with Geomagnetic Activity in Human Subjects
Related Links:
2019 ARV Session Calendar
An Interpretation of the Fields of Force and How they are Utilized in Culture and for ARV accuracy
LST Seasonal Precognition Calendar
The Solar Institute’s Remote Viewing Series
Jasmine, Cosmic Rays and the Human Nervous System
ARV Session Configuration Calendar
ARV Sessions are based upon 3 Parameters -
Seasonal LST Peaks
Favorable Moon Phase
A Quiet Magnetometer & Calm Schuman Resonance
Seasonal LST Peaks
Because all ARV sessions are conducted around 13:30LST, the conductivity of the fields varies throughout the year. It does have cycles with a peak in spring at midnight, as shown in the LST precognition calendar.
Favorable Moon Phase
ARV sessions peak around the full moon, which is a time that the moon is inside earths magnetometer . This occurs 3 days before a full moon and 6 days after the full moon.
A Quiet Magnetometer & Calm Schuman Resonance
A disturbed Magnetometer is the result of disturbances in earth's geomagnetic field. This has a collective effect which affects all people on earth. I have devoted an entire article to this which can be read here.
When solar wind speed conditions are favorable (in the 350 to 400 range) the following ARV schedule can be constructed -
LST Seasonal Peaks during Spring and Summer - ARV Sessions are practiced outside of the Favorable Moon Phase as long as the magnetometer is calm and quiet.
Non-LST Seasonal Peaks - ARV Sessions are practiced during a Quiet Magnetometer & Calm Schuman Resonance 6 days from a full moon until 6 days after the full moon
Favorable Moon Phases - During non-LST Seasonal Peaks, ARV sessions are conducted 6 days before and after a full moon as long as the magnetometer is calm and quiet.
Solar Flares - When solar flares & sunspots are both occuring together and the magnetometer is quiet.
Note - The ARV Countdown Page should be checked daily in case any of the above solar weather conditions occur. If they do, the countdown time and date will be re-set to reflect the new solar weather conditions, resulting in a new ARV session date.
Plotting Future Solar Activity for Favorable ARV Sessions
The period before higher geomagnetic disturbances and an increase in the solar wind - which is a period ARV accuracy is enhanced, is usually, but not always, associated with solar flares. This is because disturbances in earth's geomagnetic activity occur a few days after a solar flare as highly charged particles impact earth's magnetosphere. Hence, if the sun's 10.7cm flux shows a forecasted rise occurring before a large increase in geomagnetic activity, it may mean that a solar flare will occur during the increase in 10.7cm flux activity. Another window of peak ARV session accuracy occurs just after higher solar activity and can be plotted by watching when AP values are forecasted to decline, which is often accompanied by quiet magnetometer activity.Using terrestrial Weather to Plot Solar Flares
While this method is not always accurate, it can help to narrow down the best date(s) for ARV sessions. Because abrupt weather changes can sometimes cause the 10.7 cm radio flux to become disturbed, as I show in this article, it sometimes indicates future solar flare activity because solar activity influences the weather. Hence looking at the terrestrial weather in the days ahead can give a general idea of the pattern of future solar activity. As solar activity begins to calm down, it is often accompanied by a peak in barometric air pressure. Hence looking for these peaks can give one clues to times solar activity is optimal for successful ARV sessions.
Links
LST Sidereal Clock