Step 1: GENERATE YOUR REQUEST

Your run results will be published online under your Run Registration Number (FirstName_LastName_MMDDYY_ModelType_RunNumber) e.g. John_Smith_032511_SH_1.

WORK OR SCHOOL EMAILhow to contact you

Enter a valid work or school email address

FIRST NAME (GIVEN)*your given name

Enter your given name

LAST NAME (FAMILY)*your family name

Enter your family name

RUN NUMBER* max of 4 runs per day

choose run number for today 1 2 3 4 Unless you want to overwrite it

KEYWORD/S* helps to sort and search the results of the tomographic runs

Enter a keyword

Step 2: SET THE 3D RECONSTRUCTION TIME INTERVAL

Interplanetary scintillation (IPS) data from STElab (Nagoya University, Japan) used as an input to the Heliospheric Tomography Model are generally available from year 1997 (CR 1918) through the present time.
DATA OUTAGES:
- Years 1997-2009 had regular outages of data from December to May. From late 2010 the scintillation-level (density proxy) data coverage has been year-round (no Dec-May outages).
- There are no data for almost all of the year 2010 (through November).
- There are some short duration data outages due to typhoons.

OPTION 1Carrington Rotation

cr

choose carrington rotation2131213021292128212721262125212421232122212121202119211821172116211521142113211221112110210921082107210621052104210321022101210020992098209720962095209420932092209120902089208820872086208520842083208220812080207920782077207620752074207320722071207020692068206720662065206420632062206120602059205820572056205520542053205220512050204920482047204620452044204320422041204020392038203720362035203420332032203120302029202820272026202520242023202220212020201920182017201620152014201320122011201020092008200720062005200420032002200120001999199819971996199519941993199219911990198919881987198619851984198319821981198019791978197719761975197419731972197119701969196819671966196519641963196219611960195919581957195619551954195319521951195019491948194719461945194419431942194119401939193819371936193519341933193219311930192919281927192619251924192319221921192019191918

OPTION 2 Date of Interest

year

choose year2012201120102009200820072006200520042003200220012000199919981997

month

choose month January February March April May June July August September October November December

day

choose day12345678910111213141516171819202122232425262728293031

RUN DURATIONfixed

Step 3: SELECT THE SOURCE OF IN-SITU INPUT DATA TO MATCH THE REMOTE-SENSING DATA NEAR EARTH

(e.g., Jackson et al., 2012, Solar Phys., DOI 10.1007/s11207-012-0102-x)
When selecting the time interval above please take into account additional specific in-situ data availability restrictions below. Please note that there are additional short in-situ input data gaps (such as during shock events) not mentioned for each data set.

NO in-situ input data(A 3.3/cc density mean is assumed at 1 AU)

ACE level 0Available 1998 through now

ACE level 2Avail. 1998 to 2010-10-09

CELIASAvail. 1997 to 2025-02-11. Data gap: 1998-06-24 to 1998-10-29.

WINDAvail. 1997 to about 2025-02-11

ONLY if you require a customized simulation setup not provided by the standard submission options. Unlike the standard runs that are automatically processed, special requests are reviewed and manually modified by the CCMC staff. Please note that special requests are reviewed and manually modified by the CCMC staff and are executed only if resources are available.

DETAILSbrief description of your special request