Question 1:
Does the word 'suite' as used in Section 10.3 refer only to the named 'suites' in Table 10.4? There is ambiguity in Table 10.4. For example, the energetic particles 'Package' could also be called a 'suite'.
Also, there is no 'Fields suite' at the European level (that is, the RPW and MAG instruments are entirely separate - in terms of hardware and management).
Response to Question 1:
The sum of all the flight components of a Principal Investigator’s proposal is a “suite.” A suite may contain one or more instruments. The “suite” is equivalent to an instrument package; that is, each row of Table 10-4 is an instrument suite.
Question 2:
Can we have clarification of 'joint design' as used in Section10.3? Exactly what is precluded? Can we consider an instrument design which includes contributions of flight hardware subsystems from US and European?
Response to Question 2:
“Joint design” refers to a situation where there is not a clean interface, and an identifiable U.S. deliverable depends upon design information from a non-U.S. partner. An example of a joint design is a U.S. investigator providing flight software to a
non-U.S. hardware provider; the software provider requires significant interaction and exchange of design details with the non-U.S. provider to complete the U.S. deliverable. In the example, the “what” that is being provided requires more than interface
definition and control documentation; it also requires the definition and exchange of “how” the design is executed on both sides of the interface. The lack of a clean interface (or “joint design”) involves the exchange of design details that may not be
allowed by International Traffic in Arms Regulations or Export Administration Regulations.
An instrument design that includes contributions of flight hardware subsystems from U.S. and European co-Investigators where clean interfaces exist is permitted.
Question 3:
What does NASA consider to be a 'sensor?' Is this a statement about interfaces? For example, would a US telescope with a clean interface to a European detector array be considered a sensor?
Response to Question 3:
The “sensor” is defined in section 10.3 as an instrument suite that has a non-U.S. Principal Investigator and has a U.S. flight contribution with a clean interface. The “sensor” term is exclusively associated with a non-U.S. Principal Investigator.
A U.S. telescope with a clean interface to a European detector array where the Principal Investigator is from Europe is a “sensor.” If the U.S. telescope has a European detector array and the Principal Investigator is from the U.S., the combined
telescope and detector array are termed an “instrument” in the solicitation.
Question 4:
There is repeated reference to opportunities for NASA-funded PIs to lead development of Instrument "suites", and that ESA member states may provide "sensors" for NASA-led instrument "suites" (i.e. Table 10-1).
However, not all of the potential NASA-led investigations are actually "suites", but stand-alone "instruments". In this case, is it correct and acceptable to interpret Table 10-1 as "NASA provides instruments; ESA member states
may provide components or subsystems for NASA-led instruments."
Response to Question 4:
In the case where NASA is the lead agency, it is correct and acceptable to interpret Table 10-1 as “NASA provides instruments; ESA member states may provide components or subsystems for NASA-led instruments provided that a clean
interface is maintained between the contributions from NASA and the ESA member states.”
Question 5:
Section 10.1.3 (Available NASA resources) states that "the total cost to NASA for all FOSO investigations selected through this AO from Phase A to E is approximately $65M in "real year" dollars...". However, all other elements of the
SMEX AO are solicited in "FY08 dollars". Given this fact for the over-arching SMEX AO, are the available funds for the FOSO investigations actually in "FY08 dollars", and not "Real Year dollars"?
Response to Question 5:
Costs for FOSO investigations should be stated in real year dollars. The FOSO amendment provides exceptions to the SMEX AO for the FOSO proposals.
Question 6:
Section 10.3 (Types of Proposals) states that "Proposals that provide for "joint design" of an instrument with a non-US partner are not solicited or appropriate". What constitutes a "joint-design"? Are component and/or subsystem
contributions from non-US partners to a NASA-led investigation allowed? Are I&T, calibration, and mission/science ops activities provided by non-US partners allowed?
Response to Question 6:
“Joint design” refers to a situation where there is not a clean interface, and an identifiable U.S. deliverable depends upon design information from a non-U.S. partner. An example of a joint design is a U.S. investigator providing flight
software to a non-U.S. hardware provider; the software provider requires significant interaction and exchange of design details with the non-U.S. provider to complete the U.S. deliverable. In the example, the “what” that is being provided
requires more than interface definition and control documentation; it also requires the definition and exchange of “how” the design is executed on both sides of the interface. The lack of a clean interface (or “joint design”) involves the
exchange of design details that may not be allowed by International Traffic in Arms Regulations or Export Administration Regulations.
An instrument design that includes contributions of flight hardware subsystems from U.S. and European co-Investigators where clean interfaces exist is permitted. For example, a European telescope with a U.S. detector array is permitted,
because the no knowledge of “how” the detectors or telescopes are developed or manufactured is required to interface the telescope and detectors; only knowledge of the interface is required. Integration and test are only allowed when knowledge
of the design details of all the contributed components is not needed to perform the integration.
The U.S.-provided items on European-led instruments as well as the U.S.-led instruments will deliver a data acceptance package when the item is delivered; therefore, items should not plan to be shipped to Europe several times prior to final
delivery. Calibration on U.S.-provided items should occur prior to final delivery and should not require shipment to Europe several times prior to final delivery.
All instruments/instrument suites will be integrated with the spacecraft in Europe, and comprehensive performance testing of the observatory is expected to be performed in Europe after integration of the instruments with the spacecraft bus.
The Principal Investigator for a U.S.-led instrument/instrument suite should plan to support integration and comprehensive performance testing in Europe. ESA will perform mission operations for the observatory. The Principal Investigator
of each instrument/instrument suite is expected to lead the science operations; science operations support from non-U.S. participants is permitted.
Question 7:
Section 10.2.2 (Solar Orbiter Mission) states that "the reference trajectory will bring the observatory as close as about 0.22 AU by the end of the transfer phase". However, the HELEX STDT report states that the perihelion distance is 0.28 AU.
The perihelion distance is an important mission design parameter which has significant impact on instrument design due to the heat load seen by each instrument. Which perihelion distance should potential proposers design to?
Response to Question 7:
The HELEX STDT report is incorrect. The correct statement is, “the reference trajectory will bring the observatory as close as about 0.22 AU by the end of the transfer phase.”
Question 8:
Section 10.4.2 (Cost Requirements and Funding Policies) states that "for the purpose of this AO, an adequate unencumbered reserve on the PI Mission Cost is measured against the cost to complete through Phases A-F, and is a minimum
of 30% including funded schedule reserve". What is the reserve policy for NASA-led FOSO instruments with international hardware contributions? Does reserve against the international contributions need to be held "in addition to"
the 30% unencumbered reserve?
Response to Question 8:
International contributions are permitted under a “no exchange of funds” provision. It should be assumed that the international contribution carries its own adequate reserves. Unencumbered reserves apply only to the portion of the mission
funded by this AO.
Question 9:
What is the classification for an instrument responding to the Focused Opportunity for Solar Orbiter (FOSA)? For SMEX, Section 4.4.2 defines the Class D Payload Classification and also refers to the SMEX MAR document. ESA documents
referenced for Solar Orbiter seem typical of a Class A or Class B requirement since mission life is approximately 9 years.
Response to Question 9:
The Risk Category for instruments and sensors proposed to the FOSO is Risk Category C as defined in NASA Procedural Requirements (NPR) 8705.4 due to the lifetime of the Solar Orbiter mission. NPR 8705.4 is available at
http://nodis3.gsfc.nasa.gov/.
Question 10:
Please clarify and provide us with a copy of the Mission Assurance Requirements (MAR) for Solar Orbiter. You also reference the Solar Orbiter MAR in table 10-6 “Responsibilities of the PI of a FOSO Investigation”.
Response to Question 10:
The Solar Orbiter MAR has not been baselined, but its content will be very similar to the Geospace-Radiation Belt Storm Probes (G-RBSP) Program Mission Assurance Requirements (MAR). The G-RBSP MAR should be used in place of the
Solar Orbiter MAR. Note that the G-RBSP mission is a Risk Category C mission as defined in NPR 8705.4.
Question 11:
Section 10.2 Reference Payload states that the “Nominal accommodation of all instruments has been defined with the exception of a wide-field heliospheric imager. With the caveats mentioned in the previous paragraph, it is anticipated that the
available resources for a wide angle coronagraph/heliospheric imager will be in the range of 5-10 kilograms in mass, 5-10 Watts in power, and a telemetry bandwidth of ~20 kilobits per second.” In section 3.6.3 of the ESA Payload Definition
Document (PDD), there is a chart that defines the instrument accommodation maximum resources as slightly different. Which document (the SMEX AO Addendum or the ESA PDD) should we consider as the master for developing our proposal concept?
Response to Question 11:
The FOSO Amendment to the SMEX AO takes precedence over the ESA PDD.
Question 12:
The FOSO does not specify volume constraints for the Heliospheric Imager (HI) instrument; however it does anticipate a resource allocation from ESA documents. The ESA PDD specifies a volume of 400 x 250 x 200 mm3 and a projected
footprint of no more than 400 x 250 mm2. If we keep the total volume the same, may we change some of the dimensions of the footprint or review changes to these dimensions in an accommodation study as long as we are close to these desired values?
Response to Question 12:
Changes to the dimensions or projected footprint may be proposed, but the proposer should be mindful of the limited resources available on the Solar Orbiter.
Question 13:
Section 3.6.3.2 of ESA’s Payload Definition Document, shows the Heliospheric Imager instrument mounted to the same side as a solar panel in figure 3.6.2. Straylight from the solar array makes it extremely difficult to meet filed of view
requirements associated with the Heliospheric Imager. During the accommodation study, would ESA consider moving the solar panels to another plane while keeping the Heliospheric Imager instrument in the ram or anti-ram side and on the ecliptic plane?
Response to Question 13:
Moving the solar panels may be considered during an accommodation study.
Question 14:
In section 3.6 of the ESA Payload Definition Document and in section 3.4 of the ESA Experiment Interface Document (EID); it is not clear from the information whether an externally mounted Heliospheric Imager type instrument would have
access to cold or hot patches as required for our thermal accommodation. The ESA EID states, “Units requiring special exposure to the space environment are mounted outside the spacecraft body. They are thermally decoupled from the
spacecraft structure and therefore thermally controlled by the unit itself.” Would ESA allow any re-consideration of these constraints in the accommodation study for the instruments since the thermal designs presented in the Annex 11 show
considerable accommodations in both the heat shield and suggest cold/hot patches for thermal interfacing (reference page 16 of EADS-Astrium presentation)?
Response to Question 14:
Reconsideration of the constraints may be considered during an accommodation study.
Question 15:
For proposals submitted against the FOSO, are just the cost tables B3 etc. required, or is a full proposal required?
Response to Question 15:
A full proposal that includes the cost tables is required.
Question 16:
Is it true that Solar Orbiter proposal can only be submittd to the FOSO? What about an instrument that is responsive to the ESA Payload Defintion Document but not the HELEX Report?
Response to Question 16:
It is true that a Solar Orbiter proposal can only be submitted to the FOSO instead of having the option to submit the proposal to either the SMEX or FOSO opportunities. The science prioritization in the
HELEX report takes precedence over the prioritization in the ESA Payload Definition Document; however, all FOSO proposals will be judged on scientific merit in addition to the other evaluation factors
specified in paragraph 10.6.1.
Question 17:
Is it possible to propose a SMEX MO for a sensor or instrument for Solar Orbiter? Can they then use Risk Category D instead of C for Solar Orbiter?
Response to Question 17:
Solar Orbiter proposals must be submitted to the FOSO instead of to the SMEX MO. The Risk Category C was established for Solar Orbiter due to the five-year prime mission life and 4.5 year
extended lifetime.
Question 18: (Modified 01.25.2008)
Can NASA provide clarification as to what, if anything, that has been requested by ESA in the Solar Orbiter AO is to be included in a proposal to NASA under the FOSO amendment. We assume that the due
date for any such submission is Feb 1, 2008. Is that correct? Are there any submissions by US PIs directly to ESA? If so can that be done by the US PI submitting to NASA and then NASA forwarding the documents to ESA?
Can NASA provide further clarification as to whether there are any submissions by US PIs directly to ESA Solar Orbiter AO?
Response to Question 18:
ESA has not requested that any specific content be in the FOSO proposals, but we have coordinated the dates in the FOSO Amendment with ESA before releasing the FOSO Amendment.
It is not appropriate for U.S. PIs to submit proposals directly to ESA, and NASA will not forward proposals to ESA. Instead, NASA will use the evaluation criteria defined in the
FOSO to determine the best science; after categorization of the U.S. proposals, NASA will coordinate proposed selections with ESA. U.S. investigators who want to collaborate on investigations that are led by a PI from an ESA member state should
coordinate the content of their U.S. proposals informally with the PI from the ESA member state before submitting their proposals to the FOSO, and the FOSO proposal should be for U.S. funding only. U.S. PIs who want to include contributions
from non-U.S. investigators should informally coordinate the collaboration before submitting the PI proposal for U.S. funding to the FOSO, and the non-U.S. investigators should propose to either the ESA AO or to their governments.
Please note that A. 18 has been modified . The partial sentence stating that "It is not appropriate for U.S. PIs to submit proposals directly to ESA" has been removed.
Furthermore, proposers may send proposals to ESA. It is their choice and NASA is not requiring it. However, proposers must obey US export control law. Proposers should also check the ESA Solar Orbiter
AO and the
Q&A pages for updates.
Question 19:
The FOSO states that the wide angle coronagraph/heliospheric imager fulfills the science linkage between Solar Orbiter and the Sentinels Mission. Can you please provide the orbits of the four Sentinels (location and time), so that we may
compare the Sentinels locations with the Solar Orbiter fields of view?
Response to Question 19:
We have attached the orbit files for 4 Sentinels spacecraft to be launched on March 29, 2017. Please keep in mind that this date necessarily is not the final launch date. These are plain ASCII files with simple headers.
The multiple Venus encounter orbits are provided as examples only. While they are valid flight dynamics solutions, modifications of the orbit parameters are possible. Please note that the orbit data are presented in a
Sun MOJ2000 heliocentric solar equatorial inertial coordinate system, therefore Earth is moving in this representation. To facilitate planning efforts, Earth and Venus orbit files are also included in the same coordinate system.
Question 20:
According to the ESA web site, it would appear that they are expecting US investigators to submit to ESA as well as NASA. This is not mentioned in the FOSO or the SMEX AO, and it could cause some ITAR problems. Is there any
guidance on this?
Response to Question 20:
U.S. investigators should only submit their proposals to the FOSO. NASA will coordinate the results of the evaluations of the selectable U.S. proposals with ESA prior to NASA selection. The ESA proposal should briefly describe
the NASA contribution, and the proposal to NASA should describe the complete NASA contribution. NASA will manage the development of the U.S. contributions to avoid ITAR problems.