Table 2.
Experiments with their data-taking periods and associated expected Solar modulation level.
| Experiment (period) | ϕprior | Reference |
|---|---|---|
| [MV] | ||
| Li/C and B/C (“Base”) | ||
| AMS-02 (’11/05-’16/05) | 676 | Aguilar et al. (2018) |
| ACE-CRIS (’97/08-’98/04) | 528 | Lave et al. (2013) |
| ACE-CRIS (’98/01-’99/01) | 582 | de Nolfo et al. (2006) |
| ACE-CRIS (’01/05-’03/09) | 872 | Lave et al. (2013) |
| ACE-CRIS (’09/03-’10/01) | 445 | Lave et al. (2013) |
| IMP8 (’74/01-’78/10) | 540 | Garcia-Munoz et al. (1987) |
| ISEE3-HKH (’78/08-’81/04) | 742 | Krombel & Wiedenbeck (1988) |
| Ulysses-HET (’90/10-’95/07) | 732 | Duvernois et al. (1996) |
| Voyager1&2 (’77/01-’98/12) | 450 | Lukasiak (1999) |
| Be/B data | ||
| AMS-02 (’11/05-’16/05) | 676 | Aguilar et al. (2018) |
| 10Be/Be data | ||
| IMP7&8 (’72/09-’75/09) | 543 | Garcia-Munoz et al. (1977) |
| IMP7&8 (’74/01-’80/05) | 580 | Garcia-Munoz et al. (1981) |
| ISEE3-HKH (’78/08-’79/08) | 653 | Wiedenbeck & Greiner (1980) |
| Ulysses-HET (’90/10-’97/12) | 661 | Connell (1998) |
| Voyager1&2 (’77/01-’98/12) | 450 | Lukasiak (1999) |
| 10Be/9Be data | ||
| Most precise low-energy data (“ACE”) | ||
| ACE-CRIS (’97/08-’99/07) | 581 | Yanasak et al. (2001) |
| ACE-SIS (’97/08-’99/07) | 581 | Yanasak et al. (2001) |
| Remaining low-energy data (“LE w/o ACE”) | ||
| IMP7&8 (’74/01-’80/05) | 580 | Garcia-Munoz et al. (1981) |
| ISEE3-HKH (’78/08-’79/08) | 653 | Wiedenbeck & Greiner (1980) |
| Ulysses-HET (’90/10-’97/12) | 661 | Connell (1998) |
| Voyager1&2 (’77/01-’98/12) | 450 | Lukasiak (1999) |
| Intermediate energy | ||
| ISOMAX (’98/08) | 618 | Hams et al. (2004) |
| Preliminary data (Appendix B only) | ||
| PAMELA (’06/07-’14/09) | 500 | Bogomolov & Vasilyev (2019) |
Notes. In the list below, datasets from the same experiment and data taking periods share a common Solar modulation level in the analyses. PAMELA data are from a preliminary analysis. For this reason, they are never considered in our main results, and are only used for illustration in Appendix B.
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