2.3.0 spase://GBO/NumericalData/NeutronMonitor/Huancayo/PT1H Cosmic Ray Intensities Hourly averages from the Huancayo Neutron Monitor Huancayo Hourly Counting Rates 2021-04-26T14:44:18Z Hourly averages of relativistic cosmic ray intensities from the Huancayo Neutron Monitor Please acknowledge the Principal Investigator (Dr. Clifford Lopate) spase://SMWG/Person/Clifford.Lopate PrincipalInvestigator DataProducer World Data Center for Cosmic Rays (WDCCR) Read_Me (Starting Point of Data Access) https://cidas.isee.nagoya-u.ac.jp/WDCCR/readme.html This Web page includes numerical data and plots of cosmic-ray neutron observations covering the interval from 1953 to present. spase://VEPO/NumericalData/NeutronMonitor/Huancayo/PT1H spase://SMWG/Repository/WDC/CosmicRays/NagoyaU Online Open Huancayo hourly intensities http://cr0.izmiran.ru/huan/main.htm Parent directory containing compressed yearly files with naming convention "File: HuancayoYYYY" containing hourly averaged Huancayo neutron monitor intensity measurements for YYYY = 1953 through 1992. Text C. Lopate, University of New Hampshire spase://SMWG/Instrument/NeutronMonitor/Huancayo EnergeticParticles 1953-01-01T00:00:00.000 1992-12-31T23:59:59.000 PT1H Heliosphere.NearEarth Interval Start Time Columns 1 - 3 Nominal Start Time for the average given as MM/DD/YYYY HH SSSSSSSSSS where MM = month of year (01-12) DD = Day of Month (01-31) YYYY = Gregorian Year AD HH = Hour of Day (00-23) SSSSSSSSSS = Seconds since 00:00:00 Jan. 01, 1904 PT1H Temporal Huancayo Hourly Average Column 4 Huancayo pressure corrected counts per hour, prescaled by 100 Periods with no data are indicated by -1.0 For true counts per hour, the value given must be multiplied by 100. Corrections for geomagnetic drift affecting the cutoff have not been applied PT1H (counts/hr) 0 100000 -1.0 Proton Integral Counts 12.92 1.0E6 GV Huancayo Cutoff Drift Corrected Hourly Average Column 5 Huancayo counts per hour, prescaled by 100 and corrected for pressure and geomagnetic cutoff drift due to secular changes in the geomagnetic field. Periods with no data are indicated by -1.00 For true counts per hour, the value given must be multiplied by 100. PT1H (counts/hr) 0 100000 -1.00 Proton Integral Counts 12.92 1.0E6 GV