Science
ACTUAL PROBLEMS OF AVIATION AND AEROSPACE SYSTEMS
Kazan Daytona Beach


To 50-th Anniversary of Yu.A.Gagarin flight

and in Memory of Prof. Luigi Broglio, Founder of University satellites Program

Luigi Broglio and the San Marco satellites

Filippo Graziani, Ugo Ponzi

Engineering Aerospace School, Sapienza University of Rome

This article has two chapters. First chapter is prepared by Prof.F.Graziani. In this one it is highlighted the role and place of Engineering Aerospace School of Sapienza University of Rome in Space research Programs from 1961. Also it is presented short description about 1-st  IAA Conference on University satellite missions and CUBESAT Workshop. Second chapter is prepared by Prof. Ugo Ponzi on paper materials. This is highlighting the merit of works and Person of Prof. Luigi Broglio, who is Founder of Program and San Marco Project with brilliant idea about Universities small satellites.

I. Introducing Chapter

Engineering Aerospace School of Sapienza University of Rome and Conferences

on Universities satellites

The Engineering Aerospace School of Sapienza University of Rome is honoured to host the 1st IAA Conference on University Satellites Missions and the 1stCubesat Winter Workshop, dedicated to the new generation of university satellites: micro, pico, femtosatellites, from cubesats to pocketsats. In particular the 1st Cubesat Winter Workshop will provide the opportunity to students to have an overview of the current status of the university microsatellites, as well as to exchange different points of view through a variety of sessions, laboratories and forums.

We are also very proud to recall that the Engineering Aerospace School itself initiated the university satellite program, exactly fifty years ago.

In fact, the year 2011 marks the 50th Anniversary of the beginning of the Piloted Astronautics Era: on April 12th, 1961, Soviet cosmonaut Yury Gagarin orbited the Earth! And another important event occurred on that very same time.

During the COSPAR session, held in Florence that year, where the Russian space representatives announced the breaking news:"The first human in outer space", our very own Professor Luigi Broglio, Dean of the Engineering Aerospace School for over thirty five years, invited some of his dear American colleagues and friends to dinner. And while having dinner that night, he proposed a joint program to investigate upper-air density and associated ionosphere phenomena related to the solar activity in the equatorial region, using small satellites.

"You are brave" said the Americans, and then readily continued "we will support you". The idea of the San Marco Project was hence born!

The activity on small satellite design, manufacture and integration involving Professors and Researchers of the Engineering Aerospace School of Sapienza University of Rome, therefore began, based on the suggestions and supervision of the Nasa people. An important operational objective was to establish since 1967 a mobile launch capability in a equatorial region (Kenya) to carry out mainly direct low equatorial orbits by using efficiently a mid-size vehicle.

Small satellites at that time meant 150 kg of weight, but compared to today's miniaturized components can be easily scaled at least to one order of magnitude less!

The Conference and the Workshop are directed also to both past and present students already skilled and experienced in satellite design and manufacture, as well as to beginner students for which special laboratories will be organized during the workshop, and last but not least to future students (high school students) for which a full half-day meeting is specially dedicated.

Professors and Industry Representatives are warmly invited to offer their experience and valuable support to the young people attending this workshop.

Moreover, since Conference and the Workshop are inserted in the memorial week dedicated to the memory of Professor Luigi Broglio (1911-2001), all participants are invited to see the films on the San Marco Project (San Marco satellites and San Marco Equatorial Range in Kenya).

Also, off the beaten track tourist walks in the streets of Ancient Roma will be organized, as we wish that the glorious past history of Roma and the prestigious future projects of the Astronautical Era can mix together in the present Conference on University Satellites Missions and Cubesat Workshop!

The low cost of developing and launching a CubeSat has opened the possibility of bringing CubeSats as educational tools into the classrooms of many universities and even some high schools. Unlike larger projects, the short development time for CubeSats of typically two years from initial design to launch is very compatible with the duration of Master and PhD theses. As educational hands-on projects CubeSats are ideal and it is, therefore, no surprise that the CubeSat community is rapidly growing. The CubeSat standard was defined in 1999 by Stanford University and California Polytechnic State University. Now, only 10 years later, about 200 CubeSats worldwide have already been launched or are in different stages of development.

Industry is also getting involved by launching CubeSats for technological applications, by developing and selling CubeSat subsystems and deployers and offering launch services. Space agencies and other institutions are using CubeSats for biological, microgravity and re-entry research. More and more large rocket companies are beginning to cater for the needs of this emerging new market segment. A number of CubeSats can be equipped with common instruments and launched, deployed and operated together as a distributed sensor network for atmospheric or space weather research, for Earth environment monitoring or ship identification and tracking at very low cost.

Each year, numerous conferences in different parts of the world are organized which include CubeSat sessions. However, there are currently only two workshops which are dedicated to CubeSats and are held every year on a regular basis. These are the CubeSat Developers' Workshop in April in San Luis Obispo in California and the CubeSat Developers' Summer Workshop in August in Logan, Utah.

The Education Office of the European Space Agency (ESA) organized a Vega Maiden Flight CubeSat Workshop on 22-24 January 2008 at ESTEC in the Netherlands. The Workshop was the first of its kind at European level and gathered almost all of the European CubeSat teams together for the first time. The Workshop was attended by over 140 participants, and 24 CubeSat teams from 13 European countries presented their CubeSat designs. While the Workshop was dedicated to the flight opportunity of the Vega Maiden Flight, many participants expressed an interest in having an annual workshop in Europe to bring the European CubeSat community together on a regular basis for further information exchange and fostering a network of cooperating institutes in this area. A year later, on 20-22 January 2009, the Second European CubeSat Workshop was organized by ESA's Education Office at ESTEC and was attended by 190 participants.

Nowadays, there are an estimated 100 universities in 30 European countries interested in developing CubeSats and there is, therefore, clearly a need for continuing this series of European CubeSat conferences. The 1st CubeSat Winter Workshop in Europe on 24-29 January 2011 in Rome is the third in the series, the European CubeSat Symposium on 30 January-1 February 2012 in Brussels will be the fourth in the series. The conferences in Rome and Brussels and future conferences in this series will be held at the end of January each year and will be jointly organized by the University of Rome, ESA's Education Office and the von Karman Institute for Fluid Dynamics.

II. Main Chapter

The San Marco Project

First and foremost let me express a warm note of thanks to the organizers who, while planning the topics of the Conference on university satellite missions, elected to reserve time for L.Broglio and the San Marco satellites notwithstanding their "space age antiquity".

But it is just this remoteness that is one of the many merits accompanying their achievements: that is, the merit of being ahead, with the activities of the San Marco Project, of any other Italian initiative of this type and of trail-blazing a path to the first effective operation of Italian universities in this field.

In addition to this primogeniture, one must underscore the fact that it was not an operation of scientific or technological content limited to just one sector but rather a comprehensive achievement that dealt with the fundamental requirements of space activity, tackling and solving the knotty problems associated with design, construction, ground testing and launch of satellites as well as the related satellite data acquisition.

In fact, the effort deployed at that time was directed at establishing also a base in Kenya (the San Marco Range equipped with launch structures, and satellite control and telemetry instrumentation), a Center in Rome with installations and laboratories for satellite development and environmental tests - namely, Centro Ricerche Aerospaziali (CRA) located on Via Salaria, destined to become in time the current Centro di Ricerca Progetto San Marco (CRPSM ) - and training and organizing the personnel of various specializations assigned to the operations in the above named sites.

What was achieved back then and the results we are still gleaning - partly thanks to the introduction of fresh resources - allows us to state that, on the whole, the activities carried out by the San Marco Project reached a magnitude as yet unsurpassed by any other space-dedicated Italian university structure.

What were the results obtained?

Let me list a few significant ones:

-       the first Italian scientific satellite (San Marco 1) injected into orbit in December 1964. So, Italy preceded all other European countries, next only to the USSR and USA;

-       the subsequent satellites SM 2, 3, 4 and 5 were also built by CRA. They were launched from San Marco Range, that is, the first space base in the world established at low latitude (Kenya) which became operational in 1967 with the first direct equatorial orbit;

-       hospitality offered by said SM satellites to NASA and German experiments to the end of establishing a broad investigative capability into the statics and dynamics of neuter and ionized atmosphere;

-       the achievement claimed by the so-called "Balance" (of which more details later on) as an original instrument for in situ measuring of aerodynamic drag;

-       the success of San Marco Range as an ideal Base capable of launching small scientific satellites exploiting as much as possible the capabilities of the launch vehicle, and the geomagnetic and radiative peculiarities at the Equator;

-       the orbital launches from San Marco Range of four NASA scientific satellites and a UK one (it was the first time that NASA devolved such a function to another country);

-       the use of the Range ground structures for scientific activity in support to other Italian, European, US and Chinese missions that could avail themselves of San Marco Stations control, command and telemetry capabilities;

-       development of studies on fundamental remote sensing methodologies and the resultant  applications of data thus acquired for land management activities and natural resources monitoring;

-       last but not least, the great impulse imparted to the renovation of didactics within the School of Aerospace Engineering of the University "La Sapienza".

The importance acquired by the use of the above mentioned structures even recently results from  the  wide spectrum of cooperative relationships instituted by San Marco Project with many of the world's main players in the field of space activities.

L.Broglio's figure and professional life

Whenever I pause to ponder over such numerous and compelling achievements - both in terms of contents and precocity with respect to other space operators, be it Italy or Europe - I cannot help remembering and renovating my admiration for the figure of Luigi Broglio who, of all this, was the promoter and whose birth centenary falls this year while his demise occurred in this month, a decade ago.

L.Broglio's life and the history of the San Marco Project are so interrelated that it will be easy in this venue to proceed to a commemoration of his accomplishments by just retracing the main steps of the Project itself. Bearing in mind, however, that although the constraints of time will force me to illustrate him as the protagonist of this glorious undertaking, I certainly do not mean to detract from him the great number of his other accomplishments that rightly made him a distinguished scientist and Teacher.

By now, everybody is in agreement that L.Broglio was indeed the Father of the Italian space activity. And if we consider Space as a summation of all the elements that constitute and manifest it (that is to say, the disciplines that nourish it, the technological means that support it down to the applications that realize it), please allow me to say in no uncertain terms that L.Broglio deserves this recognition because of the way he successfully operated ahead of his contemporaries in each of these areas.

L.Broglio's academic and military careers were with no doubt decisive for his entering the field of space activities with such far-reaching actions.

As a teacher and Principal of the School of Aerospace Engineering that he restructured  in 1963, L.Broglio had the opportunity to concern himself with a number of fundamental topics of space culture: aeronautics and rocketry, with in-depth studies of structure mechanics and heat transmission problems, aero-elastic and aero-thermodynamic similarities, astrodynamics and re-entry problems, as well as theoretical and experimental research on high atmosphere motions. And so he arrived at original scientific results of great importance that were the fruit of his intellectual vivacity, of an unusual culture coupled with the acuteness of his analyses and the immediate perception of the essential aspects of the problems at issue.

L.Broglio used to aim at results of a concrete nature and useful for applications, as it happened for example in the 50's with his "Method of Balanced Forces" whereby, at a time when computers were unknown, the mathematical model of aeronautical structures not sufficiently restrained (wings) was conformed to the convergence requirements characteristic of successive approximation methods. Or, among many other instances, his elegant treatment of boundary conditions and of non-linearity in Space/Time problems of thermal conduction in bodies subjected to convective and radiative heating.

Concurrently, L.Broglio was a brilliant officer of the Air Force Engineer Corps whose pinnacle he reached at the end of his career, gaining the esteem of the High Command and the priceless support that the Italian Air Force would contribute to the successive operational phases of the San Marco Project.

It is safe to assume that the symbiosis between University and Armed Forces - that enabled the San Marco Project to reach such relevant objectives - was a comparison of collaboration that, I presume, was never again attained with such amplitude. All this was possible because of L.Broglio's numerous insights: he was indeed able to put to good use the positions reached in the execution of his military and academic duties, after perceiving ahead of time the realities of space and identifying the practicable paths that could get round the obstacles.

Nowadays, cooperation in space activities under bilateral or international agreements is a recurring fact among major space players. Fifty years ago was this indeed the formula arrived at intuitively by L.Broglio to govern his relationship with NASA.

Birth of the San Marco Project

At that time L.Broglio had developed at the School of Aerospace Engineering remarkable operational capabilities in the sectors of advanced aeronautical research and rocketry, and was about to bridge a few gaps so as to enable his group to play in the immediate future an effective role in space activities. It was necessary to absorb and study in depth the elements of the new culture, to be able to design and develop satellites, have a vehicle for injection into orbit, own a launch base and staff it with specialized personnel.

Italy had neither space vehicles nor an adequate launch base. That being so, L.Broglio, on the strength of a successful sounding rocket launch campaign, asked NASA to make available a US vehicle and proposed a cooperative program under which Italy would supply:

-       a satellite with a scientific objective of great relevance at the time (in situ measurement of atmospheric density at orbital altitudes by means of an innovative instrumentation);

-       a launch Base, likewise conceptually original, capable of launching satellites into direct equatorial orbits;

-       personnel experienced in launch techniques and readily available for further training on the vehicle.

His proposal, approved by NASA whose decision fell for LTV's Scout vehicle, had the backing of the Italian Air Force, National Research Council (CNR), and national Government that allocated the necessary funds.

In essence this was the content of a "Memorandum of Understanding" signed in 1962 by Vice-President Johnson for the US and by the Italian Minister for Foreign Affairs.

The Agreement opened a phase of close cooperation in the scientific and technological fields between NASA and CRA. This cooperation lasted for more than thirty years and had a considerable political weight since it was for long the major space cooperation program between the two countries.

Originality of the satellite mission

Entering into that Agreement L.Broglio contributed with original ideas that enabled Italy to be on equal terms with the counterpart.

The first mission included an Italian experiment - promptly accepted by NASA - that was indeed a piece of further evidence of the way L.Broglio managed to conceive solutions conceptually appropriate when the objective was difficult to achieve because of absence or insufficiency of technological supports.

At that time measurements of high-altitude atmospheric density were carried out by in-situ ionization sensors sadly characterized by poor accuracy. Otherwise, an indirect method was used that was based on the aerodynamic force  F= CDrV2/2 arrived at by the variation of orbital parameters astride a long series of satellite passes, but the end result was only averaged out data.

L.Broglio's intuition was instead that of obtaining direct measurements of aerodynamic force by means of the so-called "Balance" placed on board the satellite.

To do this, it became necessary to configure the satellite in two parts that were capable of sliding with respect to each other.

-       an internal heavy body containing all on board instrumentation;

-       an external shell secured to the central body with an elastic joint.

The aerodynamic force acting upon the shell was measured by detecting the deformation of the elastic joint.

It is therefore worth noting that it was not an accelerometer, in which the sensor is subjected to its own inertial force, but rather an oscillating two-mass system where the force to be measured acts directly on the lesser mass (shell) as would be the case in a dynamometer.

The concept was straightforward but its practical application presented a few arduous engineering problems that needed solving.

Because the satellite was spin-stabilized, it became obviously necessary to have the CG of the internal body coincide with the CG of the shell, and house the elastic element in this point.

Moreover, to obtain favorable measuring conditions it was necessary for the shape of the shell to be at least axial-symmetric with respect to the spin axis or, still better, spherical so as to reduce the aerodynamic force down to a simple resistance regardless of the satellite attitude.

The balance instrument

At first, in order for the elastic joint to be sensitive to forces and insensitive to momentum, we made use of three linear elements with one degree of freedom, placed in series at 90° to each other in the direction of the satellite body axes. As a result, joint deformation was decomposed automatically in the three components along the axes and measured as the relative displacement between the two rigid bases of each of the three linear elements. The joint thus conceived and designed was called "Balance" by analogy with the balances/scales used in aerodynamic tunnels. The number of linear elements could be reduced to two if the spin axis remained constantly perpendicular to velocity. In the history of San Marco satellites, the transition to a two-component system only took place when the control system was able to maintain said required attitude with great accuracy. The utilization of a pair of linear elements on each axis made it possible to attain a complete symmetry of mass also with regard to the mechanical parts of the Balance.

The measurement of deformations, that is, the displacement δ between the two bases of each linear element was obtained using differential transformer-type sensors. Mounted in pairs to each element, they could also compensate automatically for the effect produced by ever possible thermal deformations.

The study of the Balance response to forces variable over time was conducted using a three-body mathematical model (central body, shell, rigid coupling between the two measuring groups x and y). For example, in the case of San Marco 5 satellite the minimum natural frequency ω0 was equal to 15.88 rad/s. In view of the actual value of spin velocity equal to Ωsp = 0.628 rad/s, the ratio Ωsp/ω0 = 0.04 demonstrates that the Balance responded in a static way to the modulation induced by the satellite rotation. In addition, because the response may be considered still flat for an excitation with frequency ω¢ such that the value ω¢/ω0 is not greater than about 0.2, it followed that the Balance was able to investigate phenomena with frequency ω¢= 0.2ω0 = 3.2 rad/s still responding statically.

Which corresponds to a resolution power relative to a path along the orbit given by S=2πV/ω¢= 15.7 km (that is to say, 2750 samplings for an orbit with Perigee at 200 km and Apogee at 600 km).

The satellite Project

The shell was required to be very light with respect to the internal body, which also points out the advantage of the model used (San Marco model) over the accelerometer.

The satellite design, that put into practice L.Broglio's original concept, satisfied its particular requirements of function and configuration thanks to a series of solutions, the principal instances of which are only briefly mentioned here:

-       the spherical shape of the shell was obtained by using truncated cones pieced together so as to facilitate the insertion of mica "windows" for illumination of the solar cells mounted to the internal body and more openings around the shell to allow installation of mechanical elements (satellite side supports, antennas, inertia booms mounted to the internal body) or access to attitude sensors and other on board instruments;

-       installation of the Balance to the satellite internal body and shell in the two poles of the latter using cylindrical axial arms designed such as to cross the shell in a contact-free way; the same "no contact" positioning applied to the support of the internal body attachment flange too;

-       device to block the motion of the internal body relative to the shell, active from completion of assembly to injection for protection of the Balance;

-       addition of four articulated arms on plane x y to recover a ratio of inertia Iz /Ix= Iz /Iy compatible with the stability of the spin motion.

The same figure shows the satellite SM 5 with some of its characteristics. Worthy of note is the high value of mass density due to the requirement to accommodate into internal body of the satellite NASA and DLVR instruments that went along with the Balance. They were an Airglow Solar Spectrometer for solar and interplanetary radiation; a Wind and Temperature Spectrometer for neutral particles components and kinetic temperature; six Electric Field Sensors (EFI) for the electric field components. Because of the presence of EFI (provided with four retractable wires with terminal masses with functions of electrode at a distance of 20 m from the axis) it became necessary to evaluate also the interrelation of the motion of these with the motion of the satellite rigid body.

Conclusion

Here it is not analyzed all board systems, such as power supply, data handling, telemetry, attitude determination and control, which also sometimes required original solutions.

Likewise, it would be difficult to dedicate a detailed chapter to the scientific results obtained by the Balance and other experiments.

Therefore, to complete this outline of L.Broglio's achievements in the framework of the scientific objective of the satellite mission, which we have only begun to describe, let me just say that in the whole series of San Marco satellites his intuition, that is, the Italian experiment of the Balance, turned out to be completely functional to the objective, supplying very interesting results for the study of quasi-static and dynamic conditions of the high atmosphere in the belt from 140 to 600 km of altitude.

Exhaustive evidence of this may be drawn for example by the comparison results, that show the correspondence between thermospheric phenomena/orbital events and the Balance response.

With this last brief mention of L.Broglio's scientific merits, I hope to have completed - however summarily - the portrait of a personage who was undoubtedly exceptional, and well-deserving, for the Italian academic world and the Country.

A personage who did not confine himself to transmit to others his far-seeing ideas but who, rather, led from the front and saw them through till the successful achievement of difficult objectives that aroused the world's scientific interest.

It was a long, hard journey but L.Broglio could set out on it because he was also endowed with great human qualities that I have not had the possibility to mention so far, that is, the courage to take upon himself the onus of heavy responsibilities vis-à-vis the Government and the Country's public opinion, the tenacity and faith in his work.

And I think I would do him wrong if, next to him, I were not to mention the large group of San Marco Project collaborators, each of whom deserves our deep gratitude.

It is impossible to remember all of them. I will therefore confine myself to mentioning my departed colleagues: Professor Giorgio Ravelli and Professor Carlo Arduini, with whom I shared the responsibility of satellites design and development, and Professor Michele Sirinian who led the organization and execution of the orbital launches.



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